Aerosol-cloud interaction Anatoli Bogdan Institute of Physical Chemistry, University of Innsbruck Austria and Department of Physics, University of Helsinki.

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Aerosol-cloud interaction

Anatoli Bogdan

Institute of Physical Chemistry University of Innsbruck Austria

andDepartment of Physics University of Helsinki

Finland

Contents

- role of aerosol in cloud formation - ideal gas - vapor pressure and partial vapor pressure - Kelvin equation - hygroscopic aerosol particles - Raoultrsquos law - Kohler curves

Cloud condensation nuclei or CCNs or cloud seeds are small particles (typically 02 microm or 1100 th the size of a cloud droplet) about which cloud droplets coalesce Water requires a non-gaseous surface to make the transition from a vapor to a liquid In the atmosphere this surface presents itself as tiny solid or liquid particles called CCNs When no CCNs are present water vapor can be supercooled below 0degC before droplets spontaneously form

At T gt 0 ordmC the air would have to be supersaturated to ~400 before the droplets could form The concept of cloud condensation nuclei has led to the idea of cloud seeding that tries to encourage rainfall by seeding the air with condensation nuclei It has further been suggested that creating such nuclei could be used for marine cloud brightening a geo-engineering technique

Aerosol pollution over Northern India and Bangladesh - NASA

httpenwikipediaorgwikiCloud_condensation_nuclei

httpearthobservatorynasagovFeaturesAerosols

Warm Clouds

Warm clouds consist entirely of droplets which have been formed by condensation onto aerosol particles Aerosol particles respond to changes in humidity in different ways depending on their chemical composition and solubility Particles which are soluble or hydrophilic take on water as humidity increases and increase in size

Above a certain relative humidity soluble particles will deliquesce ndash the solid particle dissolves in the water it has taken on and becomes a tiny liquid drop but not yet a cloud drop For many soluble salts deliquescence happens at relative humidity around 60 ndash 80 These droplets exist in equilibrium with water vapor in the surrounding air

The growth of such particles with increase in relative humidity is expressed by the Koumlhler equation and is a function of the size and chemical composition of the particle

Prior to the consideration of the Kohler aquation we will firstly consider several important notions needed for the understanding of the matter

General about gases and vapors

Perfect gas

Atmosphere is a mixture of gases Prier to the study of the real atmosphere (a mixture of real gases) we firstly will consider a notion of perfect (ideal) gas Gas under very small pressure (le 1 atm) is a very good approximation of perfect gas

In perfect gas i) the distance between molecules is much larger than the length of free

path of molecules and ii) the interaction between molecules is restricted only to their collisions

which are considered to be similar to that of the hard balls

Thus in the perfect gas the molecules possess only kinetic energy whereas potential energy of interaction between the molecules is absent As a result internal energy E of perfect gas is independent on pressure and volume E ne E (p V) Internal energy is determined only by the kinetic motion of molecules and can be easily changed by the addition (or withdrawing) of heat ie by changing its temperature Thus E =E (T)

Vapor pressure of water

Above the surface of liquid water there always exists some amount of vapor and consequently there is a vapor pressure When a container containing water is open then the number of the escaping molecules is larger than the number of molecules coming back from the vaporphase (Fig 1) In this case water vapor pressure is small and far from saturation

The atmosphere is a mixture of gases including water vapor

When the container is closed then the water vapor pressure above the surface increases (concentration of molecules increases) and therefore the number of molecules coming back increases too (Fig2)

After a while the number of molecules escaping the liquid and those coming back becomes equal Such situation is called by dynamic equilibrium between the escaping and returning molecules (Fig 3) In this case the water vapor pressure over the liquid water is called saturated water pressure

Saturated water vapor pressure is a function of temperature only and independent on the presence of other gases

The temperature dependence is exponential In the case of water vapor the semi empirical dependence reads as

DTTCT

BA

sw ep

ln

where temperature is in Kelvin and A = 7734 B = -7235 C = - 82 D = 0005711

132 Air humidity Amount of water vapor in the air can be expressed by several different ways

Specific humidity Mass of water vapor per unit mass of humid air air

OH

m

m 2

Absolute humidity Mass of water vapor per unit volume of humid air (kgm3) Relative humidity (RH) Ratio of water vapor pressure pw to the saturated water vapor pressure at that temperature multiplied by 100

RH = 100)(

Tp

ppure

ws

w (153)

Saturation ratio S Ratio

S =)( Tp

ppure

ws

w (154)

From the last two definitions we see that RH = S100 ie their physical meanings are almost the same Supersaturation S - 1 gt 0

For the perfect gas a following (experimental) equation of state p = f (T V n) is true

pV= nNAkbT (11) where p is pressure V volume n number of moles NA Avogadro number kb

Boltzmann constant and T temperature in Kelvin Since kb NA = R (gas constant) for the amount of gas of one mole (n = 1) the equation of state (11) can be written as

pV = RT (12) Using simple kinetic theory of gases and Newtonrsquos laws of motion one can show (see for example Understanding Physics (1998) p 249 or Hinds (1982) pp 15-16) that

pV = RT = KE = 3

2Nmmol (13)

where KE is kinetic energy of the molecules composing the perfect gas mmol mass of

molecule N number of molecules and 2 average of square of molecular velocities (see below) The expression (13) means that the kinetic energy KE which is also the internal energy of the perfect gas E is independent on pressure volume or molecular weight and depends only on temperature ie KE = E = E (T)

Equations derived for the perfect gas work also in the case of mixture of gases provided that the individual gases (components of the gaseous mixture) and the mixture itself behave perfectly Mathematically this means that are valid both the equations of state for each component of the gaseous mixture i

piV = niRT (17) and the equation of state for the mixture itself

pV = nRT (18) Daltonrsquos law for a mixture of perfect gases The pressure p exerted by a mixture of the perfect gases is the sum of the partial pressures pi of the gases Mathematically it reads p = sum pi (19)

Physical meaning of partial pressure According to the Daltonrsquos law for the perfect gases the pressure p exerted by a gaseous mixture is the sum of the partial pressures pi of the gases In the case of the perfect gases the partial pressure pi is simply the pressure which the gas would exert if it occupied the container alone at the same temperature But in the case of the real gases at moderate pressures the interaction between molecules of different gases makes the total pressure being slightly different (smaller) from the simple sum of the pressures of the gas components if they were alone Therefore for the real gas the partial pressure pi of the gas component i in the gaseous mixture is defined as pi = Xi p (115) where p is the total pressure of the mixture(Compare (115) with (110)) It follows from Eqs (19) and (115) that p = (X1 + X2 + X3 + ) p = p1 + p2 + p3 + = sum pi (116) ie similar for the mixture of the perfect gases the sum of the partial pressures of real gases is also equal to the total pressure of the mixture (But total pressure of the mixture of the perfect gases is not equal to that of the real gases)

Kelvin equation

ps(r) ps(infin) = exp (2 σwρwRvTr) = exp (ar)r = droplet radius

ps(r) = the actual vapour pressure of droplet of radius r

ps(infin)= the saturation vapour pressure over bulk water

σw = surface tension

ρw= water density

Rv - the universal gas constant T - temperature

ExampleSaturation ratio Critical radius 1 012 μm11 00126 μm2 173 nm

What is going on with soluble aerosol particles for example such which are composed of NaCl sea salt ammonium sulfate etc

Hygroscopy is the ability of a substance to attract water molecules from the atmosphere through either absorption or adsorption

Hygroscopic substances include sugar honey glycerol ethanol methanol sulfuric acid many salts and many other substances

Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

All soluble salts will deliquesce if the air is sufficiently humid

141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

AA

A Xp

p or pA = XA pA (160)

The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

Koumlhler Curve = Kelvin equation + Raoultrsquos law

p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

The critical radius rc and critical supersaturation Sc are calculated as

rc= (3ba)12 and Sc= (4 a3[27 b])12

httpenwikipediaorgwikiFileKohler_curvespng

Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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    Contents

    - role of aerosol in cloud formation - ideal gas - vapor pressure and partial vapor pressure - Kelvin equation - hygroscopic aerosol particles - Raoultrsquos law - Kohler curves

    Cloud condensation nuclei or CCNs or cloud seeds are small particles (typically 02 microm or 1100 th the size of a cloud droplet) about which cloud droplets coalesce Water requires a non-gaseous surface to make the transition from a vapor to a liquid In the atmosphere this surface presents itself as tiny solid or liquid particles called CCNs When no CCNs are present water vapor can be supercooled below 0degC before droplets spontaneously form

    At T gt 0 ordmC the air would have to be supersaturated to ~400 before the droplets could form The concept of cloud condensation nuclei has led to the idea of cloud seeding that tries to encourage rainfall by seeding the air with condensation nuclei It has further been suggested that creating such nuclei could be used for marine cloud brightening a geo-engineering technique

    Aerosol pollution over Northern India and Bangladesh - NASA

    httpenwikipediaorgwikiCloud_condensation_nuclei

    httpearthobservatorynasagovFeaturesAerosols

    Warm Clouds

    Warm clouds consist entirely of droplets which have been formed by condensation onto aerosol particles Aerosol particles respond to changes in humidity in different ways depending on their chemical composition and solubility Particles which are soluble or hydrophilic take on water as humidity increases and increase in size

    Above a certain relative humidity soluble particles will deliquesce ndash the solid particle dissolves in the water it has taken on and becomes a tiny liquid drop but not yet a cloud drop For many soluble salts deliquescence happens at relative humidity around 60 ndash 80 These droplets exist in equilibrium with water vapor in the surrounding air

    The growth of such particles with increase in relative humidity is expressed by the Koumlhler equation and is a function of the size and chemical composition of the particle

    Prior to the consideration of the Kohler aquation we will firstly consider several important notions needed for the understanding of the matter

    General about gases and vapors

    Perfect gas

    Atmosphere is a mixture of gases Prier to the study of the real atmosphere (a mixture of real gases) we firstly will consider a notion of perfect (ideal) gas Gas under very small pressure (le 1 atm) is a very good approximation of perfect gas

    In perfect gas i) the distance between molecules is much larger than the length of free

    path of molecules and ii) the interaction between molecules is restricted only to their collisions

    which are considered to be similar to that of the hard balls

    Thus in the perfect gas the molecules possess only kinetic energy whereas potential energy of interaction between the molecules is absent As a result internal energy E of perfect gas is independent on pressure and volume E ne E (p V) Internal energy is determined only by the kinetic motion of molecules and can be easily changed by the addition (or withdrawing) of heat ie by changing its temperature Thus E =E (T)

    Vapor pressure of water

    Above the surface of liquid water there always exists some amount of vapor and consequently there is a vapor pressure When a container containing water is open then the number of the escaping molecules is larger than the number of molecules coming back from the vaporphase (Fig 1) In this case water vapor pressure is small and far from saturation

    The atmosphere is a mixture of gases including water vapor

    When the container is closed then the water vapor pressure above the surface increases (concentration of molecules increases) and therefore the number of molecules coming back increases too (Fig2)

    After a while the number of molecules escaping the liquid and those coming back becomes equal Such situation is called by dynamic equilibrium between the escaping and returning molecules (Fig 3) In this case the water vapor pressure over the liquid water is called saturated water pressure

    Saturated water vapor pressure is a function of temperature only and independent on the presence of other gases

    The temperature dependence is exponential In the case of water vapor the semi empirical dependence reads as

    DTTCT

    BA

    sw ep

    ln

    where temperature is in Kelvin and A = 7734 B = -7235 C = - 82 D = 0005711

    132 Air humidity Amount of water vapor in the air can be expressed by several different ways

    Specific humidity Mass of water vapor per unit mass of humid air air

    OH

    m

    m 2

    Absolute humidity Mass of water vapor per unit volume of humid air (kgm3) Relative humidity (RH) Ratio of water vapor pressure pw to the saturated water vapor pressure at that temperature multiplied by 100

    RH = 100)(

    Tp

    ppure

    ws

    w (153)

    Saturation ratio S Ratio

    S =)( Tp

    ppure

    ws

    w (154)

    From the last two definitions we see that RH = S100 ie their physical meanings are almost the same Supersaturation S - 1 gt 0

    For the perfect gas a following (experimental) equation of state p = f (T V n) is true

    pV= nNAkbT (11) where p is pressure V volume n number of moles NA Avogadro number kb

    Boltzmann constant and T temperature in Kelvin Since kb NA = R (gas constant) for the amount of gas of one mole (n = 1) the equation of state (11) can be written as

    pV = RT (12) Using simple kinetic theory of gases and Newtonrsquos laws of motion one can show (see for example Understanding Physics (1998) p 249 or Hinds (1982) pp 15-16) that

    pV = RT = KE = 3

    2Nmmol (13)

    where KE is kinetic energy of the molecules composing the perfect gas mmol mass of

    molecule N number of molecules and 2 average of square of molecular velocities (see below) The expression (13) means that the kinetic energy KE which is also the internal energy of the perfect gas E is independent on pressure volume or molecular weight and depends only on temperature ie KE = E = E (T)

    Equations derived for the perfect gas work also in the case of mixture of gases provided that the individual gases (components of the gaseous mixture) and the mixture itself behave perfectly Mathematically this means that are valid both the equations of state for each component of the gaseous mixture i

    piV = niRT (17) and the equation of state for the mixture itself

    pV = nRT (18) Daltonrsquos law for a mixture of perfect gases The pressure p exerted by a mixture of the perfect gases is the sum of the partial pressures pi of the gases Mathematically it reads p = sum pi (19)

    Physical meaning of partial pressure According to the Daltonrsquos law for the perfect gases the pressure p exerted by a gaseous mixture is the sum of the partial pressures pi of the gases In the case of the perfect gases the partial pressure pi is simply the pressure which the gas would exert if it occupied the container alone at the same temperature But in the case of the real gases at moderate pressures the interaction between molecules of different gases makes the total pressure being slightly different (smaller) from the simple sum of the pressures of the gas components if they were alone Therefore for the real gas the partial pressure pi of the gas component i in the gaseous mixture is defined as pi = Xi p (115) where p is the total pressure of the mixture(Compare (115) with (110)) It follows from Eqs (19) and (115) that p = (X1 + X2 + X3 + ) p = p1 + p2 + p3 + = sum pi (116) ie similar for the mixture of the perfect gases the sum of the partial pressures of real gases is also equal to the total pressure of the mixture (But total pressure of the mixture of the perfect gases is not equal to that of the real gases)

    Kelvin equation

    ps(r) ps(infin) = exp (2 σwρwRvTr) = exp (ar)r = droplet radius

    ps(r) = the actual vapour pressure of droplet of radius r

    ps(infin)= the saturation vapour pressure over bulk water

    σw = surface tension

    ρw= water density

    Rv - the universal gas constant T - temperature

    ExampleSaturation ratio Critical radius 1 012 μm11 00126 μm2 173 nm

    What is going on with soluble aerosol particles for example such which are composed of NaCl sea salt ammonium sulfate etc

    Hygroscopy is the ability of a substance to attract water molecules from the atmosphere through either absorption or adsorption

    Hygroscopic substances include sugar honey glycerol ethanol methanol sulfuric acid many salts and many other substances

    Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

    Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

    All soluble salts will deliquesce if the air is sufficiently humid

    141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

    AA

    A Xp

    p or pA = XA pA (160)

    The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

    Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

    The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

    The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

    Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

    Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

    p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

    wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

    Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

    Koumlhler Curve = Kelvin equation + Raoultrsquos law

    p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

    wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

    The critical radius rc and critical supersaturation Sc are calculated as

    rc= (3ba)12 and Sc= (4 a3[27 b])12

    httpenwikipediaorgwikiFileKohler_curvespng

    Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

    As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

    Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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      Cloud condensation nuclei or CCNs or cloud seeds are small particles (typically 02 microm or 1100 th the size of a cloud droplet) about which cloud droplets coalesce Water requires a non-gaseous surface to make the transition from a vapor to a liquid In the atmosphere this surface presents itself as tiny solid or liquid particles called CCNs When no CCNs are present water vapor can be supercooled below 0degC before droplets spontaneously form

      At T gt 0 ordmC the air would have to be supersaturated to ~400 before the droplets could form The concept of cloud condensation nuclei has led to the idea of cloud seeding that tries to encourage rainfall by seeding the air with condensation nuclei It has further been suggested that creating such nuclei could be used for marine cloud brightening a geo-engineering technique

      Aerosol pollution over Northern India and Bangladesh - NASA

      httpenwikipediaorgwikiCloud_condensation_nuclei

      httpearthobservatorynasagovFeaturesAerosols

      Warm Clouds

      Warm clouds consist entirely of droplets which have been formed by condensation onto aerosol particles Aerosol particles respond to changes in humidity in different ways depending on their chemical composition and solubility Particles which are soluble or hydrophilic take on water as humidity increases and increase in size

      Above a certain relative humidity soluble particles will deliquesce ndash the solid particle dissolves in the water it has taken on and becomes a tiny liquid drop but not yet a cloud drop For many soluble salts deliquescence happens at relative humidity around 60 ndash 80 These droplets exist in equilibrium with water vapor in the surrounding air

      The growth of such particles with increase in relative humidity is expressed by the Koumlhler equation and is a function of the size and chemical composition of the particle

      Prior to the consideration of the Kohler aquation we will firstly consider several important notions needed for the understanding of the matter

      General about gases and vapors

      Perfect gas

      Atmosphere is a mixture of gases Prier to the study of the real atmosphere (a mixture of real gases) we firstly will consider a notion of perfect (ideal) gas Gas under very small pressure (le 1 atm) is a very good approximation of perfect gas

      In perfect gas i) the distance between molecules is much larger than the length of free

      path of molecules and ii) the interaction between molecules is restricted only to their collisions

      which are considered to be similar to that of the hard balls

      Thus in the perfect gas the molecules possess only kinetic energy whereas potential energy of interaction between the molecules is absent As a result internal energy E of perfect gas is independent on pressure and volume E ne E (p V) Internal energy is determined only by the kinetic motion of molecules and can be easily changed by the addition (or withdrawing) of heat ie by changing its temperature Thus E =E (T)

      Vapor pressure of water

      Above the surface of liquid water there always exists some amount of vapor and consequently there is a vapor pressure When a container containing water is open then the number of the escaping molecules is larger than the number of molecules coming back from the vaporphase (Fig 1) In this case water vapor pressure is small and far from saturation

      The atmosphere is a mixture of gases including water vapor

      When the container is closed then the water vapor pressure above the surface increases (concentration of molecules increases) and therefore the number of molecules coming back increases too (Fig2)

      After a while the number of molecules escaping the liquid and those coming back becomes equal Such situation is called by dynamic equilibrium between the escaping and returning molecules (Fig 3) In this case the water vapor pressure over the liquid water is called saturated water pressure

      Saturated water vapor pressure is a function of temperature only and independent on the presence of other gases

      The temperature dependence is exponential In the case of water vapor the semi empirical dependence reads as

      DTTCT

      BA

      sw ep

      ln

      where temperature is in Kelvin and A = 7734 B = -7235 C = - 82 D = 0005711

      132 Air humidity Amount of water vapor in the air can be expressed by several different ways

      Specific humidity Mass of water vapor per unit mass of humid air air

      OH

      m

      m 2

      Absolute humidity Mass of water vapor per unit volume of humid air (kgm3) Relative humidity (RH) Ratio of water vapor pressure pw to the saturated water vapor pressure at that temperature multiplied by 100

      RH = 100)(

      Tp

      ppure

      ws

      w (153)

      Saturation ratio S Ratio

      S =)( Tp

      ppure

      ws

      w (154)

      From the last two definitions we see that RH = S100 ie their physical meanings are almost the same Supersaturation S - 1 gt 0

      For the perfect gas a following (experimental) equation of state p = f (T V n) is true

      pV= nNAkbT (11) where p is pressure V volume n number of moles NA Avogadro number kb

      Boltzmann constant and T temperature in Kelvin Since kb NA = R (gas constant) for the amount of gas of one mole (n = 1) the equation of state (11) can be written as

      pV = RT (12) Using simple kinetic theory of gases and Newtonrsquos laws of motion one can show (see for example Understanding Physics (1998) p 249 or Hinds (1982) pp 15-16) that

      pV = RT = KE = 3

      2Nmmol (13)

      where KE is kinetic energy of the molecules composing the perfect gas mmol mass of

      molecule N number of molecules and 2 average of square of molecular velocities (see below) The expression (13) means that the kinetic energy KE which is also the internal energy of the perfect gas E is independent on pressure volume or molecular weight and depends only on temperature ie KE = E = E (T)

      Equations derived for the perfect gas work also in the case of mixture of gases provided that the individual gases (components of the gaseous mixture) and the mixture itself behave perfectly Mathematically this means that are valid both the equations of state for each component of the gaseous mixture i

      piV = niRT (17) and the equation of state for the mixture itself

      pV = nRT (18) Daltonrsquos law for a mixture of perfect gases The pressure p exerted by a mixture of the perfect gases is the sum of the partial pressures pi of the gases Mathematically it reads p = sum pi (19)

      Physical meaning of partial pressure According to the Daltonrsquos law for the perfect gases the pressure p exerted by a gaseous mixture is the sum of the partial pressures pi of the gases In the case of the perfect gases the partial pressure pi is simply the pressure which the gas would exert if it occupied the container alone at the same temperature But in the case of the real gases at moderate pressures the interaction between molecules of different gases makes the total pressure being slightly different (smaller) from the simple sum of the pressures of the gas components if they were alone Therefore for the real gas the partial pressure pi of the gas component i in the gaseous mixture is defined as pi = Xi p (115) where p is the total pressure of the mixture(Compare (115) with (110)) It follows from Eqs (19) and (115) that p = (X1 + X2 + X3 + ) p = p1 + p2 + p3 + = sum pi (116) ie similar for the mixture of the perfect gases the sum of the partial pressures of real gases is also equal to the total pressure of the mixture (But total pressure of the mixture of the perfect gases is not equal to that of the real gases)

      Kelvin equation

      ps(r) ps(infin) = exp (2 σwρwRvTr) = exp (ar)r = droplet radius

      ps(r) = the actual vapour pressure of droplet of radius r

      ps(infin)= the saturation vapour pressure over bulk water

      σw = surface tension

      ρw= water density

      Rv - the universal gas constant T - temperature

      ExampleSaturation ratio Critical radius 1 012 μm11 00126 μm2 173 nm

      What is going on with soluble aerosol particles for example such which are composed of NaCl sea salt ammonium sulfate etc

      Hygroscopy is the ability of a substance to attract water molecules from the atmosphere through either absorption or adsorption

      Hygroscopic substances include sugar honey glycerol ethanol methanol sulfuric acid many salts and many other substances

      Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

      Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

      All soluble salts will deliquesce if the air is sufficiently humid

      141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

      AA

      A Xp

      p or pA = XA pA (160)

      The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

      Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

      The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

      The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

      Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

      Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

      p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

      wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

      Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

      Koumlhler Curve = Kelvin equation + Raoultrsquos law

      p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

      wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

      The critical radius rc and critical supersaturation Sc are calculated as

      rc= (3ba)12 and Sc= (4 a3[27 b])12

      httpenwikipediaorgwikiFileKohler_curvespng

      Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

      As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

      Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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        At T gt 0 ordmC the air would have to be supersaturated to ~400 before the droplets could form The concept of cloud condensation nuclei has led to the idea of cloud seeding that tries to encourage rainfall by seeding the air with condensation nuclei It has further been suggested that creating such nuclei could be used for marine cloud brightening a geo-engineering technique

        Aerosol pollution over Northern India and Bangladesh - NASA

        httpenwikipediaorgwikiCloud_condensation_nuclei

        httpearthobservatorynasagovFeaturesAerosols

        Warm Clouds

        Warm clouds consist entirely of droplets which have been formed by condensation onto aerosol particles Aerosol particles respond to changes in humidity in different ways depending on their chemical composition and solubility Particles which are soluble or hydrophilic take on water as humidity increases and increase in size

        Above a certain relative humidity soluble particles will deliquesce ndash the solid particle dissolves in the water it has taken on and becomes a tiny liquid drop but not yet a cloud drop For many soluble salts deliquescence happens at relative humidity around 60 ndash 80 These droplets exist in equilibrium with water vapor in the surrounding air

        The growth of such particles with increase in relative humidity is expressed by the Koumlhler equation and is a function of the size and chemical composition of the particle

        Prior to the consideration of the Kohler aquation we will firstly consider several important notions needed for the understanding of the matter

        General about gases and vapors

        Perfect gas

        Atmosphere is a mixture of gases Prier to the study of the real atmosphere (a mixture of real gases) we firstly will consider a notion of perfect (ideal) gas Gas under very small pressure (le 1 atm) is a very good approximation of perfect gas

        In perfect gas i) the distance between molecules is much larger than the length of free

        path of molecules and ii) the interaction between molecules is restricted only to their collisions

        which are considered to be similar to that of the hard balls

        Thus in the perfect gas the molecules possess only kinetic energy whereas potential energy of interaction between the molecules is absent As a result internal energy E of perfect gas is independent on pressure and volume E ne E (p V) Internal energy is determined only by the kinetic motion of molecules and can be easily changed by the addition (or withdrawing) of heat ie by changing its temperature Thus E =E (T)

        Vapor pressure of water

        Above the surface of liquid water there always exists some amount of vapor and consequently there is a vapor pressure When a container containing water is open then the number of the escaping molecules is larger than the number of molecules coming back from the vaporphase (Fig 1) In this case water vapor pressure is small and far from saturation

        The atmosphere is a mixture of gases including water vapor

        When the container is closed then the water vapor pressure above the surface increases (concentration of molecules increases) and therefore the number of molecules coming back increases too (Fig2)

        After a while the number of molecules escaping the liquid and those coming back becomes equal Such situation is called by dynamic equilibrium between the escaping and returning molecules (Fig 3) In this case the water vapor pressure over the liquid water is called saturated water pressure

        Saturated water vapor pressure is a function of temperature only and independent on the presence of other gases

        The temperature dependence is exponential In the case of water vapor the semi empirical dependence reads as

        DTTCT

        BA

        sw ep

        ln

        where temperature is in Kelvin and A = 7734 B = -7235 C = - 82 D = 0005711

        132 Air humidity Amount of water vapor in the air can be expressed by several different ways

        Specific humidity Mass of water vapor per unit mass of humid air air

        OH

        m

        m 2

        Absolute humidity Mass of water vapor per unit volume of humid air (kgm3) Relative humidity (RH) Ratio of water vapor pressure pw to the saturated water vapor pressure at that temperature multiplied by 100

        RH = 100)(

        Tp

        ppure

        ws

        w (153)

        Saturation ratio S Ratio

        S =)( Tp

        ppure

        ws

        w (154)

        From the last two definitions we see that RH = S100 ie their physical meanings are almost the same Supersaturation S - 1 gt 0

        For the perfect gas a following (experimental) equation of state p = f (T V n) is true

        pV= nNAkbT (11) where p is pressure V volume n number of moles NA Avogadro number kb

        Boltzmann constant and T temperature in Kelvin Since kb NA = R (gas constant) for the amount of gas of one mole (n = 1) the equation of state (11) can be written as

        pV = RT (12) Using simple kinetic theory of gases and Newtonrsquos laws of motion one can show (see for example Understanding Physics (1998) p 249 or Hinds (1982) pp 15-16) that

        pV = RT = KE = 3

        2Nmmol (13)

        where KE is kinetic energy of the molecules composing the perfect gas mmol mass of

        molecule N number of molecules and 2 average of square of molecular velocities (see below) The expression (13) means that the kinetic energy KE which is also the internal energy of the perfect gas E is independent on pressure volume or molecular weight and depends only on temperature ie KE = E = E (T)

        Equations derived for the perfect gas work also in the case of mixture of gases provided that the individual gases (components of the gaseous mixture) and the mixture itself behave perfectly Mathematically this means that are valid both the equations of state for each component of the gaseous mixture i

        piV = niRT (17) and the equation of state for the mixture itself

        pV = nRT (18) Daltonrsquos law for a mixture of perfect gases The pressure p exerted by a mixture of the perfect gases is the sum of the partial pressures pi of the gases Mathematically it reads p = sum pi (19)

        Physical meaning of partial pressure According to the Daltonrsquos law for the perfect gases the pressure p exerted by a gaseous mixture is the sum of the partial pressures pi of the gases In the case of the perfect gases the partial pressure pi is simply the pressure which the gas would exert if it occupied the container alone at the same temperature But in the case of the real gases at moderate pressures the interaction between molecules of different gases makes the total pressure being slightly different (smaller) from the simple sum of the pressures of the gas components if they were alone Therefore for the real gas the partial pressure pi of the gas component i in the gaseous mixture is defined as pi = Xi p (115) where p is the total pressure of the mixture(Compare (115) with (110)) It follows from Eqs (19) and (115) that p = (X1 + X2 + X3 + ) p = p1 + p2 + p3 + = sum pi (116) ie similar for the mixture of the perfect gases the sum of the partial pressures of real gases is also equal to the total pressure of the mixture (But total pressure of the mixture of the perfect gases is not equal to that of the real gases)

        Kelvin equation

        ps(r) ps(infin) = exp (2 σwρwRvTr) = exp (ar)r = droplet radius

        ps(r) = the actual vapour pressure of droplet of radius r

        ps(infin)= the saturation vapour pressure over bulk water

        σw = surface tension

        ρw= water density

        Rv - the universal gas constant T - temperature

        ExampleSaturation ratio Critical radius 1 012 μm11 00126 μm2 173 nm

        What is going on with soluble aerosol particles for example such which are composed of NaCl sea salt ammonium sulfate etc

        Hygroscopy is the ability of a substance to attract water molecules from the atmosphere through either absorption or adsorption

        Hygroscopic substances include sugar honey glycerol ethanol methanol sulfuric acid many salts and many other substances

        Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

        Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

        All soluble salts will deliquesce if the air is sufficiently humid

        141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

        AA

        A Xp

        p or pA = XA pA (160)

        The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

        Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

        The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

        The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

        Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

        Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

        p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

        wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

        Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

        Koumlhler Curve = Kelvin equation + Raoultrsquos law

        p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

        wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

        The critical radius rc and critical supersaturation Sc are calculated as

        rc= (3ba)12 and Sc= (4 a3[27 b])12

        httpenwikipediaorgwikiFileKohler_curvespng

        Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

        As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

        Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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          Aerosol pollution over Northern India and Bangladesh - NASA

          httpenwikipediaorgwikiCloud_condensation_nuclei

          httpearthobservatorynasagovFeaturesAerosols

          Warm Clouds

          Warm clouds consist entirely of droplets which have been formed by condensation onto aerosol particles Aerosol particles respond to changes in humidity in different ways depending on their chemical composition and solubility Particles which are soluble or hydrophilic take on water as humidity increases and increase in size

          Above a certain relative humidity soluble particles will deliquesce ndash the solid particle dissolves in the water it has taken on and becomes a tiny liquid drop but not yet a cloud drop For many soluble salts deliquescence happens at relative humidity around 60 ndash 80 These droplets exist in equilibrium with water vapor in the surrounding air

          The growth of such particles with increase in relative humidity is expressed by the Koumlhler equation and is a function of the size and chemical composition of the particle

          Prior to the consideration of the Kohler aquation we will firstly consider several important notions needed for the understanding of the matter

          General about gases and vapors

          Perfect gas

          Atmosphere is a mixture of gases Prier to the study of the real atmosphere (a mixture of real gases) we firstly will consider a notion of perfect (ideal) gas Gas under very small pressure (le 1 atm) is a very good approximation of perfect gas

          In perfect gas i) the distance between molecules is much larger than the length of free

          path of molecules and ii) the interaction between molecules is restricted only to their collisions

          which are considered to be similar to that of the hard balls

          Thus in the perfect gas the molecules possess only kinetic energy whereas potential energy of interaction between the molecules is absent As a result internal energy E of perfect gas is independent on pressure and volume E ne E (p V) Internal energy is determined only by the kinetic motion of molecules and can be easily changed by the addition (or withdrawing) of heat ie by changing its temperature Thus E =E (T)

          Vapor pressure of water

          Above the surface of liquid water there always exists some amount of vapor and consequently there is a vapor pressure When a container containing water is open then the number of the escaping molecules is larger than the number of molecules coming back from the vaporphase (Fig 1) In this case water vapor pressure is small and far from saturation

          The atmosphere is a mixture of gases including water vapor

          When the container is closed then the water vapor pressure above the surface increases (concentration of molecules increases) and therefore the number of molecules coming back increases too (Fig2)

          After a while the number of molecules escaping the liquid and those coming back becomes equal Such situation is called by dynamic equilibrium between the escaping and returning molecules (Fig 3) In this case the water vapor pressure over the liquid water is called saturated water pressure

          Saturated water vapor pressure is a function of temperature only and independent on the presence of other gases

          The temperature dependence is exponential In the case of water vapor the semi empirical dependence reads as

          DTTCT

          BA

          sw ep

          ln

          where temperature is in Kelvin and A = 7734 B = -7235 C = - 82 D = 0005711

          132 Air humidity Amount of water vapor in the air can be expressed by several different ways

          Specific humidity Mass of water vapor per unit mass of humid air air

          OH

          m

          m 2

          Absolute humidity Mass of water vapor per unit volume of humid air (kgm3) Relative humidity (RH) Ratio of water vapor pressure pw to the saturated water vapor pressure at that temperature multiplied by 100

          RH = 100)(

          Tp

          ppure

          ws

          w (153)

          Saturation ratio S Ratio

          S =)( Tp

          ppure

          ws

          w (154)

          From the last two definitions we see that RH = S100 ie their physical meanings are almost the same Supersaturation S - 1 gt 0

          For the perfect gas a following (experimental) equation of state p = f (T V n) is true

          pV= nNAkbT (11) where p is pressure V volume n number of moles NA Avogadro number kb

          Boltzmann constant and T temperature in Kelvin Since kb NA = R (gas constant) for the amount of gas of one mole (n = 1) the equation of state (11) can be written as

          pV = RT (12) Using simple kinetic theory of gases and Newtonrsquos laws of motion one can show (see for example Understanding Physics (1998) p 249 or Hinds (1982) pp 15-16) that

          pV = RT = KE = 3

          2Nmmol (13)

          where KE is kinetic energy of the molecules composing the perfect gas mmol mass of

          molecule N number of molecules and 2 average of square of molecular velocities (see below) The expression (13) means that the kinetic energy KE which is also the internal energy of the perfect gas E is independent on pressure volume or molecular weight and depends only on temperature ie KE = E = E (T)

          Equations derived for the perfect gas work also in the case of mixture of gases provided that the individual gases (components of the gaseous mixture) and the mixture itself behave perfectly Mathematically this means that are valid both the equations of state for each component of the gaseous mixture i

          piV = niRT (17) and the equation of state for the mixture itself

          pV = nRT (18) Daltonrsquos law for a mixture of perfect gases The pressure p exerted by a mixture of the perfect gases is the sum of the partial pressures pi of the gases Mathematically it reads p = sum pi (19)

          Physical meaning of partial pressure According to the Daltonrsquos law for the perfect gases the pressure p exerted by a gaseous mixture is the sum of the partial pressures pi of the gases In the case of the perfect gases the partial pressure pi is simply the pressure which the gas would exert if it occupied the container alone at the same temperature But in the case of the real gases at moderate pressures the interaction between molecules of different gases makes the total pressure being slightly different (smaller) from the simple sum of the pressures of the gas components if they were alone Therefore for the real gas the partial pressure pi of the gas component i in the gaseous mixture is defined as pi = Xi p (115) where p is the total pressure of the mixture(Compare (115) with (110)) It follows from Eqs (19) and (115) that p = (X1 + X2 + X3 + ) p = p1 + p2 + p3 + = sum pi (116) ie similar for the mixture of the perfect gases the sum of the partial pressures of real gases is also equal to the total pressure of the mixture (But total pressure of the mixture of the perfect gases is not equal to that of the real gases)

          Kelvin equation

          ps(r) ps(infin) = exp (2 σwρwRvTr) = exp (ar)r = droplet radius

          ps(r) = the actual vapour pressure of droplet of radius r

          ps(infin)= the saturation vapour pressure over bulk water

          σw = surface tension

          ρw= water density

          Rv - the universal gas constant T - temperature

          ExampleSaturation ratio Critical radius 1 012 μm11 00126 μm2 173 nm

          What is going on with soluble aerosol particles for example such which are composed of NaCl sea salt ammonium sulfate etc

          Hygroscopy is the ability of a substance to attract water molecules from the atmosphere through either absorption or adsorption

          Hygroscopic substances include sugar honey glycerol ethanol methanol sulfuric acid many salts and many other substances

          Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

          Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

          All soluble salts will deliquesce if the air is sufficiently humid

          141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

          AA

          A Xp

          p or pA = XA pA (160)

          The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

          Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

          The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

          The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

          Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

          Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

          p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

          wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

          Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

          Koumlhler Curve = Kelvin equation + Raoultrsquos law

          p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

          wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

          The critical radius rc and critical supersaturation Sc are calculated as

          rc= (3ba)12 and Sc= (4 a3[27 b])12

          httpenwikipediaorgwikiFileKohler_curvespng

          Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

          As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

          Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

          • Slide 1
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          • Slide 31

            httpearthobservatorynasagovFeaturesAerosols

            Warm Clouds

            Warm clouds consist entirely of droplets which have been formed by condensation onto aerosol particles Aerosol particles respond to changes in humidity in different ways depending on their chemical composition and solubility Particles which are soluble or hydrophilic take on water as humidity increases and increase in size

            Above a certain relative humidity soluble particles will deliquesce ndash the solid particle dissolves in the water it has taken on and becomes a tiny liquid drop but not yet a cloud drop For many soluble salts deliquescence happens at relative humidity around 60 ndash 80 These droplets exist in equilibrium with water vapor in the surrounding air

            The growth of such particles with increase in relative humidity is expressed by the Koumlhler equation and is a function of the size and chemical composition of the particle

            Prior to the consideration of the Kohler aquation we will firstly consider several important notions needed for the understanding of the matter

            General about gases and vapors

            Perfect gas

            Atmosphere is a mixture of gases Prier to the study of the real atmosphere (a mixture of real gases) we firstly will consider a notion of perfect (ideal) gas Gas under very small pressure (le 1 atm) is a very good approximation of perfect gas

            In perfect gas i) the distance between molecules is much larger than the length of free

            path of molecules and ii) the interaction between molecules is restricted only to their collisions

            which are considered to be similar to that of the hard balls

            Thus in the perfect gas the molecules possess only kinetic energy whereas potential energy of interaction between the molecules is absent As a result internal energy E of perfect gas is independent on pressure and volume E ne E (p V) Internal energy is determined only by the kinetic motion of molecules and can be easily changed by the addition (or withdrawing) of heat ie by changing its temperature Thus E =E (T)

            Vapor pressure of water

            Above the surface of liquid water there always exists some amount of vapor and consequently there is a vapor pressure When a container containing water is open then the number of the escaping molecules is larger than the number of molecules coming back from the vaporphase (Fig 1) In this case water vapor pressure is small and far from saturation

            The atmosphere is a mixture of gases including water vapor

            When the container is closed then the water vapor pressure above the surface increases (concentration of molecules increases) and therefore the number of molecules coming back increases too (Fig2)

            After a while the number of molecules escaping the liquid and those coming back becomes equal Such situation is called by dynamic equilibrium between the escaping and returning molecules (Fig 3) In this case the water vapor pressure over the liquid water is called saturated water pressure

            Saturated water vapor pressure is a function of temperature only and independent on the presence of other gases

            The temperature dependence is exponential In the case of water vapor the semi empirical dependence reads as

            DTTCT

            BA

            sw ep

            ln

            where temperature is in Kelvin and A = 7734 B = -7235 C = - 82 D = 0005711

            132 Air humidity Amount of water vapor in the air can be expressed by several different ways

            Specific humidity Mass of water vapor per unit mass of humid air air

            OH

            m

            m 2

            Absolute humidity Mass of water vapor per unit volume of humid air (kgm3) Relative humidity (RH) Ratio of water vapor pressure pw to the saturated water vapor pressure at that temperature multiplied by 100

            RH = 100)(

            Tp

            ppure

            ws

            w (153)

            Saturation ratio S Ratio

            S =)( Tp

            ppure

            ws

            w (154)

            From the last two definitions we see that RH = S100 ie their physical meanings are almost the same Supersaturation S - 1 gt 0

            For the perfect gas a following (experimental) equation of state p = f (T V n) is true

            pV= nNAkbT (11) where p is pressure V volume n number of moles NA Avogadro number kb

            Boltzmann constant and T temperature in Kelvin Since kb NA = R (gas constant) for the amount of gas of one mole (n = 1) the equation of state (11) can be written as

            pV = RT (12) Using simple kinetic theory of gases and Newtonrsquos laws of motion one can show (see for example Understanding Physics (1998) p 249 or Hinds (1982) pp 15-16) that

            pV = RT = KE = 3

            2Nmmol (13)

            where KE is kinetic energy of the molecules composing the perfect gas mmol mass of

            molecule N number of molecules and 2 average of square of molecular velocities (see below) The expression (13) means that the kinetic energy KE which is also the internal energy of the perfect gas E is independent on pressure volume or molecular weight and depends only on temperature ie KE = E = E (T)

            Equations derived for the perfect gas work also in the case of mixture of gases provided that the individual gases (components of the gaseous mixture) and the mixture itself behave perfectly Mathematically this means that are valid both the equations of state for each component of the gaseous mixture i

            piV = niRT (17) and the equation of state for the mixture itself

            pV = nRT (18) Daltonrsquos law for a mixture of perfect gases The pressure p exerted by a mixture of the perfect gases is the sum of the partial pressures pi of the gases Mathematically it reads p = sum pi (19)

            Physical meaning of partial pressure According to the Daltonrsquos law for the perfect gases the pressure p exerted by a gaseous mixture is the sum of the partial pressures pi of the gases In the case of the perfect gases the partial pressure pi is simply the pressure which the gas would exert if it occupied the container alone at the same temperature But in the case of the real gases at moderate pressures the interaction between molecules of different gases makes the total pressure being slightly different (smaller) from the simple sum of the pressures of the gas components if they were alone Therefore for the real gas the partial pressure pi of the gas component i in the gaseous mixture is defined as pi = Xi p (115) where p is the total pressure of the mixture(Compare (115) with (110)) It follows from Eqs (19) and (115) that p = (X1 + X2 + X3 + ) p = p1 + p2 + p3 + = sum pi (116) ie similar for the mixture of the perfect gases the sum of the partial pressures of real gases is also equal to the total pressure of the mixture (But total pressure of the mixture of the perfect gases is not equal to that of the real gases)

            Kelvin equation

            ps(r) ps(infin) = exp (2 σwρwRvTr) = exp (ar)r = droplet radius

            ps(r) = the actual vapour pressure of droplet of radius r

            ps(infin)= the saturation vapour pressure over bulk water

            σw = surface tension

            ρw= water density

            Rv - the universal gas constant T - temperature

            ExampleSaturation ratio Critical radius 1 012 μm11 00126 μm2 173 nm

            What is going on with soluble aerosol particles for example such which are composed of NaCl sea salt ammonium sulfate etc

            Hygroscopy is the ability of a substance to attract water molecules from the atmosphere through either absorption or adsorption

            Hygroscopic substances include sugar honey glycerol ethanol methanol sulfuric acid many salts and many other substances

            Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

            Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

            All soluble salts will deliquesce if the air is sufficiently humid

            141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

            AA

            A Xp

            p or pA = XA pA (160)

            The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

            Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

            The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

            The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

            Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

            Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

            p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

            wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

            Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

            Koumlhler Curve = Kelvin equation + Raoultrsquos law

            p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

            wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

            The critical radius rc and critical supersaturation Sc are calculated as

            rc= (3ba)12 and Sc= (4 a3[27 b])12

            httpenwikipediaorgwikiFileKohler_curvespng

            Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

            As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

            Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

            • Slide 1
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              Warm Clouds

              Warm clouds consist entirely of droplets which have been formed by condensation onto aerosol particles Aerosol particles respond to changes in humidity in different ways depending on their chemical composition and solubility Particles which are soluble or hydrophilic take on water as humidity increases and increase in size

              Above a certain relative humidity soluble particles will deliquesce ndash the solid particle dissolves in the water it has taken on and becomes a tiny liquid drop but not yet a cloud drop For many soluble salts deliquescence happens at relative humidity around 60 ndash 80 These droplets exist in equilibrium with water vapor in the surrounding air

              The growth of such particles with increase in relative humidity is expressed by the Koumlhler equation and is a function of the size and chemical composition of the particle

              Prior to the consideration of the Kohler aquation we will firstly consider several important notions needed for the understanding of the matter

              General about gases and vapors

              Perfect gas

              Atmosphere is a mixture of gases Prier to the study of the real atmosphere (a mixture of real gases) we firstly will consider a notion of perfect (ideal) gas Gas under very small pressure (le 1 atm) is a very good approximation of perfect gas

              In perfect gas i) the distance between molecules is much larger than the length of free

              path of molecules and ii) the interaction between molecules is restricted only to their collisions

              which are considered to be similar to that of the hard balls

              Thus in the perfect gas the molecules possess only kinetic energy whereas potential energy of interaction between the molecules is absent As a result internal energy E of perfect gas is independent on pressure and volume E ne E (p V) Internal energy is determined only by the kinetic motion of molecules and can be easily changed by the addition (or withdrawing) of heat ie by changing its temperature Thus E =E (T)

              Vapor pressure of water

              Above the surface of liquid water there always exists some amount of vapor and consequently there is a vapor pressure When a container containing water is open then the number of the escaping molecules is larger than the number of molecules coming back from the vaporphase (Fig 1) In this case water vapor pressure is small and far from saturation

              The atmosphere is a mixture of gases including water vapor

              When the container is closed then the water vapor pressure above the surface increases (concentration of molecules increases) and therefore the number of molecules coming back increases too (Fig2)

              After a while the number of molecules escaping the liquid and those coming back becomes equal Such situation is called by dynamic equilibrium between the escaping and returning molecules (Fig 3) In this case the water vapor pressure over the liquid water is called saturated water pressure

              Saturated water vapor pressure is a function of temperature only and independent on the presence of other gases

              The temperature dependence is exponential In the case of water vapor the semi empirical dependence reads as

              DTTCT

              BA

              sw ep

              ln

              where temperature is in Kelvin and A = 7734 B = -7235 C = - 82 D = 0005711

              132 Air humidity Amount of water vapor in the air can be expressed by several different ways

              Specific humidity Mass of water vapor per unit mass of humid air air

              OH

              m

              m 2

              Absolute humidity Mass of water vapor per unit volume of humid air (kgm3) Relative humidity (RH) Ratio of water vapor pressure pw to the saturated water vapor pressure at that temperature multiplied by 100

              RH = 100)(

              Tp

              ppure

              ws

              w (153)

              Saturation ratio S Ratio

              S =)( Tp

              ppure

              ws

              w (154)

              From the last two definitions we see that RH = S100 ie their physical meanings are almost the same Supersaturation S - 1 gt 0

              For the perfect gas a following (experimental) equation of state p = f (T V n) is true

              pV= nNAkbT (11) where p is pressure V volume n number of moles NA Avogadro number kb

              Boltzmann constant and T temperature in Kelvin Since kb NA = R (gas constant) for the amount of gas of one mole (n = 1) the equation of state (11) can be written as

              pV = RT (12) Using simple kinetic theory of gases and Newtonrsquos laws of motion one can show (see for example Understanding Physics (1998) p 249 or Hinds (1982) pp 15-16) that

              pV = RT = KE = 3

              2Nmmol (13)

              where KE is kinetic energy of the molecules composing the perfect gas mmol mass of

              molecule N number of molecules and 2 average of square of molecular velocities (see below) The expression (13) means that the kinetic energy KE which is also the internal energy of the perfect gas E is independent on pressure volume or molecular weight and depends only on temperature ie KE = E = E (T)

              Equations derived for the perfect gas work also in the case of mixture of gases provided that the individual gases (components of the gaseous mixture) and the mixture itself behave perfectly Mathematically this means that are valid both the equations of state for each component of the gaseous mixture i

              piV = niRT (17) and the equation of state for the mixture itself

              pV = nRT (18) Daltonrsquos law for a mixture of perfect gases The pressure p exerted by a mixture of the perfect gases is the sum of the partial pressures pi of the gases Mathematically it reads p = sum pi (19)

              Physical meaning of partial pressure According to the Daltonrsquos law for the perfect gases the pressure p exerted by a gaseous mixture is the sum of the partial pressures pi of the gases In the case of the perfect gases the partial pressure pi is simply the pressure which the gas would exert if it occupied the container alone at the same temperature But in the case of the real gases at moderate pressures the interaction between molecules of different gases makes the total pressure being slightly different (smaller) from the simple sum of the pressures of the gas components if they were alone Therefore for the real gas the partial pressure pi of the gas component i in the gaseous mixture is defined as pi = Xi p (115) where p is the total pressure of the mixture(Compare (115) with (110)) It follows from Eqs (19) and (115) that p = (X1 + X2 + X3 + ) p = p1 + p2 + p3 + = sum pi (116) ie similar for the mixture of the perfect gases the sum of the partial pressures of real gases is also equal to the total pressure of the mixture (But total pressure of the mixture of the perfect gases is not equal to that of the real gases)

              Kelvin equation

              ps(r) ps(infin) = exp (2 σwρwRvTr) = exp (ar)r = droplet radius

              ps(r) = the actual vapour pressure of droplet of radius r

              ps(infin)= the saturation vapour pressure over bulk water

              σw = surface tension

              ρw= water density

              Rv - the universal gas constant T - temperature

              ExampleSaturation ratio Critical radius 1 012 μm11 00126 μm2 173 nm

              What is going on with soluble aerosol particles for example such which are composed of NaCl sea salt ammonium sulfate etc

              Hygroscopy is the ability of a substance to attract water molecules from the atmosphere through either absorption or adsorption

              Hygroscopic substances include sugar honey glycerol ethanol methanol sulfuric acid many salts and many other substances

              Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

              Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

              All soluble salts will deliquesce if the air is sufficiently humid

              141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

              AA

              A Xp

              p or pA = XA pA (160)

              The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

              Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

              The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

              The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

              Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

              Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

              p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

              wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

              Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

              Koumlhler Curve = Kelvin equation + Raoultrsquos law

              p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

              wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

              The critical radius rc and critical supersaturation Sc are calculated as

              rc= (3ba)12 and Sc= (4 a3[27 b])12

              httpenwikipediaorgwikiFileKohler_curvespng

              Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

              As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

              Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

              • Slide 1
              • Slide 2
              • Slide 3
              • Slide 4
              • Slide 5
              • Slide 6
              • Slide 7
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              • Slide 30
              • Slide 31

                Above a certain relative humidity soluble particles will deliquesce ndash the solid particle dissolves in the water it has taken on and becomes a tiny liquid drop but not yet a cloud drop For many soluble salts deliquescence happens at relative humidity around 60 ndash 80 These droplets exist in equilibrium with water vapor in the surrounding air

                The growth of such particles with increase in relative humidity is expressed by the Koumlhler equation and is a function of the size and chemical composition of the particle

                Prior to the consideration of the Kohler aquation we will firstly consider several important notions needed for the understanding of the matter

                General about gases and vapors

                Perfect gas

                Atmosphere is a mixture of gases Prier to the study of the real atmosphere (a mixture of real gases) we firstly will consider a notion of perfect (ideal) gas Gas under very small pressure (le 1 atm) is a very good approximation of perfect gas

                In perfect gas i) the distance between molecules is much larger than the length of free

                path of molecules and ii) the interaction between molecules is restricted only to their collisions

                which are considered to be similar to that of the hard balls

                Thus in the perfect gas the molecules possess only kinetic energy whereas potential energy of interaction between the molecules is absent As a result internal energy E of perfect gas is independent on pressure and volume E ne E (p V) Internal energy is determined only by the kinetic motion of molecules and can be easily changed by the addition (or withdrawing) of heat ie by changing its temperature Thus E =E (T)

                Vapor pressure of water

                Above the surface of liquid water there always exists some amount of vapor and consequently there is a vapor pressure When a container containing water is open then the number of the escaping molecules is larger than the number of molecules coming back from the vaporphase (Fig 1) In this case water vapor pressure is small and far from saturation

                The atmosphere is a mixture of gases including water vapor

                When the container is closed then the water vapor pressure above the surface increases (concentration of molecules increases) and therefore the number of molecules coming back increases too (Fig2)

                After a while the number of molecules escaping the liquid and those coming back becomes equal Such situation is called by dynamic equilibrium between the escaping and returning molecules (Fig 3) In this case the water vapor pressure over the liquid water is called saturated water pressure

                Saturated water vapor pressure is a function of temperature only and independent on the presence of other gases

                The temperature dependence is exponential In the case of water vapor the semi empirical dependence reads as

                DTTCT

                BA

                sw ep

                ln

                where temperature is in Kelvin and A = 7734 B = -7235 C = - 82 D = 0005711

                132 Air humidity Amount of water vapor in the air can be expressed by several different ways

                Specific humidity Mass of water vapor per unit mass of humid air air

                OH

                m

                m 2

                Absolute humidity Mass of water vapor per unit volume of humid air (kgm3) Relative humidity (RH) Ratio of water vapor pressure pw to the saturated water vapor pressure at that temperature multiplied by 100

                RH = 100)(

                Tp

                ppure

                ws

                w (153)

                Saturation ratio S Ratio

                S =)( Tp

                ppure

                ws

                w (154)

                From the last two definitions we see that RH = S100 ie their physical meanings are almost the same Supersaturation S - 1 gt 0

                For the perfect gas a following (experimental) equation of state p = f (T V n) is true

                pV= nNAkbT (11) where p is pressure V volume n number of moles NA Avogadro number kb

                Boltzmann constant and T temperature in Kelvin Since kb NA = R (gas constant) for the amount of gas of one mole (n = 1) the equation of state (11) can be written as

                pV = RT (12) Using simple kinetic theory of gases and Newtonrsquos laws of motion one can show (see for example Understanding Physics (1998) p 249 or Hinds (1982) pp 15-16) that

                pV = RT = KE = 3

                2Nmmol (13)

                where KE is kinetic energy of the molecules composing the perfect gas mmol mass of

                molecule N number of molecules and 2 average of square of molecular velocities (see below) The expression (13) means that the kinetic energy KE which is also the internal energy of the perfect gas E is independent on pressure volume or molecular weight and depends only on temperature ie KE = E = E (T)

                Equations derived for the perfect gas work also in the case of mixture of gases provided that the individual gases (components of the gaseous mixture) and the mixture itself behave perfectly Mathematically this means that are valid both the equations of state for each component of the gaseous mixture i

                piV = niRT (17) and the equation of state for the mixture itself

                pV = nRT (18) Daltonrsquos law for a mixture of perfect gases The pressure p exerted by a mixture of the perfect gases is the sum of the partial pressures pi of the gases Mathematically it reads p = sum pi (19)

                Physical meaning of partial pressure According to the Daltonrsquos law for the perfect gases the pressure p exerted by a gaseous mixture is the sum of the partial pressures pi of the gases In the case of the perfect gases the partial pressure pi is simply the pressure which the gas would exert if it occupied the container alone at the same temperature But in the case of the real gases at moderate pressures the interaction between molecules of different gases makes the total pressure being slightly different (smaller) from the simple sum of the pressures of the gas components if they were alone Therefore for the real gas the partial pressure pi of the gas component i in the gaseous mixture is defined as pi = Xi p (115) where p is the total pressure of the mixture(Compare (115) with (110)) It follows from Eqs (19) and (115) that p = (X1 + X2 + X3 + ) p = p1 + p2 + p3 + = sum pi (116) ie similar for the mixture of the perfect gases the sum of the partial pressures of real gases is also equal to the total pressure of the mixture (But total pressure of the mixture of the perfect gases is not equal to that of the real gases)

                Kelvin equation

                ps(r) ps(infin) = exp (2 σwρwRvTr) = exp (ar)r = droplet radius

                ps(r) = the actual vapour pressure of droplet of radius r

                ps(infin)= the saturation vapour pressure over bulk water

                σw = surface tension

                ρw= water density

                Rv - the universal gas constant T - temperature

                ExampleSaturation ratio Critical radius 1 012 μm11 00126 μm2 173 nm

                What is going on with soluble aerosol particles for example such which are composed of NaCl sea salt ammonium sulfate etc

                Hygroscopy is the ability of a substance to attract water molecules from the atmosphere through either absorption or adsorption

                Hygroscopic substances include sugar honey glycerol ethanol methanol sulfuric acid many salts and many other substances

                Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

                Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

                All soluble salts will deliquesce if the air is sufficiently humid

                141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

                AA

                A Xp

                p or pA = XA pA (160)

                The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

                Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

                The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

                The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

                Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

                Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

                p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

                wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

                Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

                Koumlhler Curve = Kelvin equation + Raoultrsquos law

                p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

                wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

                The critical radius rc and critical supersaturation Sc are calculated as

                rc= (3ba)12 and Sc= (4 a3[27 b])12

                httpenwikipediaorgwikiFileKohler_curvespng

                Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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                • Slide 31

                  Prior to the consideration of the Kohler aquation we will firstly consider several important notions needed for the understanding of the matter

                  General about gases and vapors

                  Perfect gas

                  Atmosphere is a mixture of gases Prier to the study of the real atmosphere (a mixture of real gases) we firstly will consider a notion of perfect (ideal) gas Gas under very small pressure (le 1 atm) is a very good approximation of perfect gas

                  In perfect gas i) the distance between molecules is much larger than the length of free

                  path of molecules and ii) the interaction between molecules is restricted only to their collisions

                  which are considered to be similar to that of the hard balls

                  Thus in the perfect gas the molecules possess only kinetic energy whereas potential energy of interaction between the molecules is absent As a result internal energy E of perfect gas is independent on pressure and volume E ne E (p V) Internal energy is determined only by the kinetic motion of molecules and can be easily changed by the addition (or withdrawing) of heat ie by changing its temperature Thus E =E (T)

                  Vapor pressure of water

                  Above the surface of liquid water there always exists some amount of vapor and consequently there is a vapor pressure When a container containing water is open then the number of the escaping molecules is larger than the number of molecules coming back from the vaporphase (Fig 1) In this case water vapor pressure is small and far from saturation

                  The atmosphere is a mixture of gases including water vapor

                  When the container is closed then the water vapor pressure above the surface increases (concentration of molecules increases) and therefore the number of molecules coming back increases too (Fig2)

                  After a while the number of molecules escaping the liquid and those coming back becomes equal Such situation is called by dynamic equilibrium between the escaping and returning molecules (Fig 3) In this case the water vapor pressure over the liquid water is called saturated water pressure

                  Saturated water vapor pressure is a function of temperature only and independent on the presence of other gases

                  The temperature dependence is exponential In the case of water vapor the semi empirical dependence reads as

                  DTTCT

                  BA

                  sw ep

                  ln

                  where temperature is in Kelvin and A = 7734 B = -7235 C = - 82 D = 0005711

                  132 Air humidity Amount of water vapor in the air can be expressed by several different ways

                  Specific humidity Mass of water vapor per unit mass of humid air air

                  OH

                  m

                  m 2

                  Absolute humidity Mass of water vapor per unit volume of humid air (kgm3) Relative humidity (RH) Ratio of water vapor pressure pw to the saturated water vapor pressure at that temperature multiplied by 100

                  RH = 100)(

                  Tp

                  ppure

                  ws

                  w (153)

                  Saturation ratio S Ratio

                  S =)( Tp

                  ppure

                  ws

                  w (154)

                  From the last two definitions we see that RH = S100 ie their physical meanings are almost the same Supersaturation S - 1 gt 0

                  For the perfect gas a following (experimental) equation of state p = f (T V n) is true

                  pV= nNAkbT (11) where p is pressure V volume n number of moles NA Avogadro number kb

                  Boltzmann constant and T temperature in Kelvin Since kb NA = R (gas constant) for the amount of gas of one mole (n = 1) the equation of state (11) can be written as

                  pV = RT (12) Using simple kinetic theory of gases and Newtonrsquos laws of motion one can show (see for example Understanding Physics (1998) p 249 or Hinds (1982) pp 15-16) that

                  pV = RT = KE = 3

                  2Nmmol (13)

                  where KE is kinetic energy of the molecules composing the perfect gas mmol mass of

                  molecule N number of molecules and 2 average of square of molecular velocities (see below) The expression (13) means that the kinetic energy KE which is also the internal energy of the perfect gas E is independent on pressure volume or molecular weight and depends only on temperature ie KE = E = E (T)

                  Equations derived for the perfect gas work also in the case of mixture of gases provided that the individual gases (components of the gaseous mixture) and the mixture itself behave perfectly Mathematically this means that are valid both the equations of state for each component of the gaseous mixture i

                  piV = niRT (17) and the equation of state for the mixture itself

                  pV = nRT (18) Daltonrsquos law for a mixture of perfect gases The pressure p exerted by a mixture of the perfect gases is the sum of the partial pressures pi of the gases Mathematically it reads p = sum pi (19)

                  Physical meaning of partial pressure According to the Daltonrsquos law for the perfect gases the pressure p exerted by a gaseous mixture is the sum of the partial pressures pi of the gases In the case of the perfect gases the partial pressure pi is simply the pressure which the gas would exert if it occupied the container alone at the same temperature But in the case of the real gases at moderate pressures the interaction between molecules of different gases makes the total pressure being slightly different (smaller) from the simple sum of the pressures of the gas components if they were alone Therefore for the real gas the partial pressure pi of the gas component i in the gaseous mixture is defined as pi = Xi p (115) where p is the total pressure of the mixture(Compare (115) with (110)) It follows from Eqs (19) and (115) that p = (X1 + X2 + X3 + ) p = p1 + p2 + p3 + = sum pi (116) ie similar for the mixture of the perfect gases the sum of the partial pressures of real gases is also equal to the total pressure of the mixture (But total pressure of the mixture of the perfect gases is not equal to that of the real gases)

                  Kelvin equation

                  ps(r) ps(infin) = exp (2 σwρwRvTr) = exp (ar)r = droplet radius

                  ps(r) = the actual vapour pressure of droplet of radius r

                  ps(infin)= the saturation vapour pressure over bulk water

                  σw = surface tension

                  ρw= water density

                  Rv - the universal gas constant T - temperature

                  ExampleSaturation ratio Critical radius 1 012 μm11 00126 μm2 173 nm

                  What is going on with soluble aerosol particles for example such which are composed of NaCl sea salt ammonium sulfate etc

                  Hygroscopy is the ability of a substance to attract water molecules from the atmosphere through either absorption or adsorption

                  Hygroscopic substances include sugar honey glycerol ethanol methanol sulfuric acid many salts and many other substances

                  Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

                  Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

                  All soluble salts will deliquesce if the air is sufficiently humid

                  141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

                  AA

                  A Xp

                  p or pA = XA pA (160)

                  The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

                  Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

                  The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

                  The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

                  Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

                  Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

                  p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

                  wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

                  Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

                  Koumlhler Curve = Kelvin equation + Raoultrsquos law

                  p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

                  wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

                  The critical radius rc and critical supersaturation Sc are calculated as

                  rc= (3ba)12 and Sc= (4 a3[27 b])12

                  httpenwikipediaorgwikiFileKohler_curvespng

                  Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                  As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                  Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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                    General about gases and vapors

                    Perfect gas

                    Atmosphere is a mixture of gases Prier to the study of the real atmosphere (a mixture of real gases) we firstly will consider a notion of perfect (ideal) gas Gas under very small pressure (le 1 atm) is a very good approximation of perfect gas

                    In perfect gas i) the distance between molecules is much larger than the length of free

                    path of molecules and ii) the interaction between molecules is restricted only to their collisions

                    which are considered to be similar to that of the hard balls

                    Thus in the perfect gas the molecules possess only kinetic energy whereas potential energy of interaction between the molecules is absent As a result internal energy E of perfect gas is independent on pressure and volume E ne E (p V) Internal energy is determined only by the kinetic motion of molecules and can be easily changed by the addition (or withdrawing) of heat ie by changing its temperature Thus E =E (T)

                    Vapor pressure of water

                    Above the surface of liquid water there always exists some amount of vapor and consequently there is a vapor pressure When a container containing water is open then the number of the escaping molecules is larger than the number of molecules coming back from the vaporphase (Fig 1) In this case water vapor pressure is small and far from saturation

                    The atmosphere is a mixture of gases including water vapor

                    When the container is closed then the water vapor pressure above the surface increases (concentration of molecules increases) and therefore the number of molecules coming back increases too (Fig2)

                    After a while the number of molecules escaping the liquid and those coming back becomes equal Such situation is called by dynamic equilibrium between the escaping and returning molecules (Fig 3) In this case the water vapor pressure over the liquid water is called saturated water pressure

                    Saturated water vapor pressure is a function of temperature only and independent on the presence of other gases

                    The temperature dependence is exponential In the case of water vapor the semi empirical dependence reads as

                    DTTCT

                    BA

                    sw ep

                    ln

                    where temperature is in Kelvin and A = 7734 B = -7235 C = - 82 D = 0005711

                    132 Air humidity Amount of water vapor in the air can be expressed by several different ways

                    Specific humidity Mass of water vapor per unit mass of humid air air

                    OH

                    m

                    m 2

                    Absolute humidity Mass of water vapor per unit volume of humid air (kgm3) Relative humidity (RH) Ratio of water vapor pressure pw to the saturated water vapor pressure at that temperature multiplied by 100

                    RH = 100)(

                    Tp

                    ppure

                    ws

                    w (153)

                    Saturation ratio S Ratio

                    S =)( Tp

                    ppure

                    ws

                    w (154)

                    From the last two definitions we see that RH = S100 ie their physical meanings are almost the same Supersaturation S - 1 gt 0

                    For the perfect gas a following (experimental) equation of state p = f (T V n) is true

                    pV= nNAkbT (11) where p is pressure V volume n number of moles NA Avogadro number kb

                    Boltzmann constant and T temperature in Kelvin Since kb NA = R (gas constant) for the amount of gas of one mole (n = 1) the equation of state (11) can be written as

                    pV = RT (12) Using simple kinetic theory of gases and Newtonrsquos laws of motion one can show (see for example Understanding Physics (1998) p 249 or Hinds (1982) pp 15-16) that

                    pV = RT = KE = 3

                    2Nmmol (13)

                    where KE is kinetic energy of the molecules composing the perfect gas mmol mass of

                    molecule N number of molecules and 2 average of square of molecular velocities (see below) The expression (13) means that the kinetic energy KE which is also the internal energy of the perfect gas E is independent on pressure volume or molecular weight and depends only on temperature ie KE = E = E (T)

                    Equations derived for the perfect gas work also in the case of mixture of gases provided that the individual gases (components of the gaseous mixture) and the mixture itself behave perfectly Mathematically this means that are valid both the equations of state for each component of the gaseous mixture i

                    piV = niRT (17) and the equation of state for the mixture itself

                    pV = nRT (18) Daltonrsquos law for a mixture of perfect gases The pressure p exerted by a mixture of the perfect gases is the sum of the partial pressures pi of the gases Mathematically it reads p = sum pi (19)

                    Physical meaning of partial pressure According to the Daltonrsquos law for the perfect gases the pressure p exerted by a gaseous mixture is the sum of the partial pressures pi of the gases In the case of the perfect gases the partial pressure pi is simply the pressure which the gas would exert if it occupied the container alone at the same temperature But in the case of the real gases at moderate pressures the interaction between molecules of different gases makes the total pressure being slightly different (smaller) from the simple sum of the pressures of the gas components if they were alone Therefore for the real gas the partial pressure pi of the gas component i in the gaseous mixture is defined as pi = Xi p (115) where p is the total pressure of the mixture(Compare (115) with (110)) It follows from Eqs (19) and (115) that p = (X1 + X2 + X3 + ) p = p1 + p2 + p3 + = sum pi (116) ie similar for the mixture of the perfect gases the sum of the partial pressures of real gases is also equal to the total pressure of the mixture (But total pressure of the mixture of the perfect gases is not equal to that of the real gases)

                    Kelvin equation

                    ps(r) ps(infin) = exp (2 σwρwRvTr) = exp (ar)r = droplet radius

                    ps(r) = the actual vapour pressure of droplet of radius r

                    ps(infin)= the saturation vapour pressure over bulk water

                    σw = surface tension

                    ρw= water density

                    Rv - the universal gas constant T - temperature

                    ExampleSaturation ratio Critical radius 1 012 μm11 00126 μm2 173 nm

                    What is going on with soluble aerosol particles for example such which are composed of NaCl sea salt ammonium sulfate etc

                    Hygroscopy is the ability of a substance to attract water molecules from the atmosphere through either absorption or adsorption

                    Hygroscopic substances include sugar honey glycerol ethanol methanol sulfuric acid many salts and many other substances

                    Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

                    Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

                    All soluble salts will deliquesce if the air is sufficiently humid

                    141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

                    AA

                    A Xp

                    p or pA = XA pA (160)

                    The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

                    Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

                    The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

                    The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

                    Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

                    Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

                    p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

                    wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

                    Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

                    Koumlhler Curve = Kelvin equation + Raoultrsquos law

                    p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

                    wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

                    The critical radius rc and critical supersaturation Sc are calculated as

                    rc= (3ba)12 and Sc= (4 a3[27 b])12

                    httpenwikipediaorgwikiFileKohler_curvespng

                    Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                    As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                    Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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                    • Slide 2
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                    • Slide 31

                      Vapor pressure of water

                      Above the surface of liquid water there always exists some amount of vapor and consequently there is a vapor pressure When a container containing water is open then the number of the escaping molecules is larger than the number of molecules coming back from the vaporphase (Fig 1) In this case water vapor pressure is small and far from saturation

                      The atmosphere is a mixture of gases including water vapor

                      When the container is closed then the water vapor pressure above the surface increases (concentration of molecules increases) and therefore the number of molecules coming back increases too (Fig2)

                      After a while the number of molecules escaping the liquid and those coming back becomes equal Such situation is called by dynamic equilibrium between the escaping and returning molecules (Fig 3) In this case the water vapor pressure over the liquid water is called saturated water pressure

                      Saturated water vapor pressure is a function of temperature only and independent on the presence of other gases

                      The temperature dependence is exponential In the case of water vapor the semi empirical dependence reads as

                      DTTCT

                      BA

                      sw ep

                      ln

                      where temperature is in Kelvin and A = 7734 B = -7235 C = - 82 D = 0005711

                      132 Air humidity Amount of water vapor in the air can be expressed by several different ways

                      Specific humidity Mass of water vapor per unit mass of humid air air

                      OH

                      m

                      m 2

                      Absolute humidity Mass of water vapor per unit volume of humid air (kgm3) Relative humidity (RH) Ratio of water vapor pressure pw to the saturated water vapor pressure at that temperature multiplied by 100

                      RH = 100)(

                      Tp

                      ppure

                      ws

                      w (153)

                      Saturation ratio S Ratio

                      S =)( Tp

                      ppure

                      ws

                      w (154)

                      From the last two definitions we see that RH = S100 ie their physical meanings are almost the same Supersaturation S - 1 gt 0

                      For the perfect gas a following (experimental) equation of state p = f (T V n) is true

                      pV= nNAkbT (11) where p is pressure V volume n number of moles NA Avogadro number kb

                      Boltzmann constant and T temperature in Kelvin Since kb NA = R (gas constant) for the amount of gas of one mole (n = 1) the equation of state (11) can be written as

                      pV = RT (12) Using simple kinetic theory of gases and Newtonrsquos laws of motion one can show (see for example Understanding Physics (1998) p 249 or Hinds (1982) pp 15-16) that

                      pV = RT = KE = 3

                      2Nmmol (13)

                      where KE is kinetic energy of the molecules composing the perfect gas mmol mass of

                      molecule N number of molecules and 2 average of square of molecular velocities (see below) The expression (13) means that the kinetic energy KE which is also the internal energy of the perfect gas E is independent on pressure volume or molecular weight and depends only on temperature ie KE = E = E (T)

                      Equations derived for the perfect gas work also in the case of mixture of gases provided that the individual gases (components of the gaseous mixture) and the mixture itself behave perfectly Mathematically this means that are valid both the equations of state for each component of the gaseous mixture i

                      piV = niRT (17) and the equation of state for the mixture itself

                      pV = nRT (18) Daltonrsquos law for a mixture of perfect gases The pressure p exerted by a mixture of the perfect gases is the sum of the partial pressures pi of the gases Mathematically it reads p = sum pi (19)

                      Physical meaning of partial pressure According to the Daltonrsquos law for the perfect gases the pressure p exerted by a gaseous mixture is the sum of the partial pressures pi of the gases In the case of the perfect gases the partial pressure pi is simply the pressure which the gas would exert if it occupied the container alone at the same temperature But in the case of the real gases at moderate pressures the interaction between molecules of different gases makes the total pressure being slightly different (smaller) from the simple sum of the pressures of the gas components if they were alone Therefore for the real gas the partial pressure pi of the gas component i in the gaseous mixture is defined as pi = Xi p (115) where p is the total pressure of the mixture(Compare (115) with (110)) It follows from Eqs (19) and (115) that p = (X1 + X2 + X3 + ) p = p1 + p2 + p3 + = sum pi (116) ie similar for the mixture of the perfect gases the sum of the partial pressures of real gases is also equal to the total pressure of the mixture (But total pressure of the mixture of the perfect gases is not equal to that of the real gases)

                      Kelvin equation

                      ps(r) ps(infin) = exp (2 σwρwRvTr) = exp (ar)r = droplet radius

                      ps(r) = the actual vapour pressure of droplet of radius r

                      ps(infin)= the saturation vapour pressure over bulk water

                      σw = surface tension

                      ρw= water density

                      Rv - the universal gas constant T - temperature

                      ExampleSaturation ratio Critical radius 1 012 μm11 00126 μm2 173 nm

                      What is going on with soluble aerosol particles for example such which are composed of NaCl sea salt ammonium sulfate etc

                      Hygroscopy is the ability of a substance to attract water molecules from the atmosphere through either absorption or adsorption

                      Hygroscopic substances include sugar honey glycerol ethanol methanol sulfuric acid many salts and many other substances

                      Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

                      Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

                      All soluble salts will deliquesce if the air is sufficiently humid

                      141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

                      AA

                      A Xp

                      p or pA = XA pA (160)

                      The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

                      Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

                      The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

                      The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

                      Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

                      Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

                      p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

                      wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

                      Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

                      Koumlhler Curve = Kelvin equation + Raoultrsquos law

                      p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

                      wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

                      The critical radius rc and critical supersaturation Sc are calculated as

                      rc= (3ba)12 and Sc= (4 a3[27 b])12

                      httpenwikipediaorgwikiFileKohler_curvespng

                      Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                      As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                      Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

                      • Slide 1
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                      • Slide 31

                        When the container is closed then the water vapor pressure above the surface increases (concentration of molecules increases) and therefore the number of molecules coming back increases too (Fig2)

                        After a while the number of molecules escaping the liquid and those coming back becomes equal Such situation is called by dynamic equilibrium between the escaping and returning molecules (Fig 3) In this case the water vapor pressure over the liquid water is called saturated water pressure

                        Saturated water vapor pressure is a function of temperature only and independent on the presence of other gases

                        The temperature dependence is exponential In the case of water vapor the semi empirical dependence reads as

                        DTTCT

                        BA

                        sw ep

                        ln

                        where temperature is in Kelvin and A = 7734 B = -7235 C = - 82 D = 0005711

                        132 Air humidity Amount of water vapor in the air can be expressed by several different ways

                        Specific humidity Mass of water vapor per unit mass of humid air air

                        OH

                        m

                        m 2

                        Absolute humidity Mass of water vapor per unit volume of humid air (kgm3) Relative humidity (RH) Ratio of water vapor pressure pw to the saturated water vapor pressure at that temperature multiplied by 100

                        RH = 100)(

                        Tp

                        ppure

                        ws

                        w (153)

                        Saturation ratio S Ratio

                        S =)( Tp

                        ppure

                        ws

                        w (154)

                        From the last two definitions we see that RH = S100 ie their physical meanings are almost the same Supersaturation S - 1 gt 0

                        For the perfect gas a following (experimental) equation of state p = f (T V n) is true

                        pV= nNAkbT (11) where p is pressure V volume n number of moles NA Avogadro number kb

                        Boltzmann constant and T temperature in Kelvin Since kb NA = R (gas constant) for the amount of gas of one mole (n = 1) the equation of state (11) can be written as

                        pV = RT (12) Using simple kinetic theory of gases and Newtonrsquos laws of motion one can show (see for example Understanding Physics (1998) p 249 or Hinds (1982) pp 15-16) that

                        pV = RT = KE = 3

                        2Nmmol (13)

                        where KE is kinetic energy of the molecules composing the perfect gas mmol mass of

                        molecule N number of molecules and 2 average of square of molecular velocities (see below) The expression (13) means that the kinetic energy KE which is also the internal energy of the perfect gas E is independent on pressure volume or molecular weight and depends only on temperature ie KE = E = E (T)

                        Equations derived for the perfect gas work also in the case of mixture of gases provided that the individual gases (components of the gaseous mixture) and the mixture itself behave perfectly Mathematically this means that are valid both the equations of state for each component of the gaseous mixture i

                        piV = niRT (17) and the equation of state for the mixture itself

                        pV = nRT (18) Daltonrsquos law for a mixture of perfect gases The pressure p exerted by a mixture of the perfect gases is the sum of the partial pressures pi of the gases Mathematically it reads p = sum pi (19)

                        Physical meaning of partial pressure According to the Daltonrsquos law for the perfect gases the pressure p exerted by a gaseous mixture is the sum of the partial pressures pi of the gases In the case of the perfect gases the partial pressure pi is simply the pressure which the gas would exert if it occupied the container alone at the same temperature But in the case of the real gases at moderate pressures the interaction between molecules of different gases makes the total pressure being slightly different (smaller) from the simple sum of the pressures of the gas components if they were alone Therefore for the real gas the partial pressure pi of the gas component i in the gaseous mixture is defined as pi = Xi p (115) where p is the total pressure of the mixture(Compare (115) with (110)) It follows from Eqs (19) and (115) that p = (X1 + X2 + X3 + ) p = p1 + p2 + p3 + = sum pi (116) ie similar for the mixture of the perfect gases the sum of the partial pressures of real gases is also equal to the total pressure of the mixture (But total pressure of the mixture of the perfect gases is not equal to that of the real gases)

                        Kelvin equation

                        ps(r) ps(infin) = exp (2 σwρwRvTr) = exp (ar)r = droplet radius

                        ps(r) = the actual vapour pressure of droplet of radius r

                        ps(infin)= the saturation vapour pressure over bulk water

                        σw = surface tension

                        ρw= water density

                        Rv - the universal gas constant T - temperature

                        ExampleSaturation ratio Critical radius 1 012 μm11 00126 μm2 173 nm

                        What is going on with soluble aerosol particles for example such which are composed of NaCl sea salt ammonium sulfate etc

                        Hygroscopy is the ability of a substance to attract water molecules from the atmosphere through either absorption or adsorption

                        Hygroscopic substances include sugar honey glycerol ethanol methanol sulfuric acid many salts and many other substances

                        Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

                        Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

                        All soluble salts will deliquesce if the air is sufficiently humid

                        141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

                        AA

                        A Xp

                        p or pA = XA pA (160)

                        The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

                        Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

                        The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

                        The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

                        Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

                        Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

                        p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

                        wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

                        Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

                        Koumlhler Curve = Kelvin equation + Raoultrsquos law

                        p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

                        wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

                        The critical radius rc and critical supersaturation Sc are calculated as

                        rc= (3ba)12 and Sc= (4 a3[27 b])12

                        httpenwikipediaorgwikiFileKohler_curvespng

                        Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                        As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                        Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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                          After a while the number of molecules escaping the liquid and those coming back becomes equal Such situation is called by dynamic equilibrium between the escaping and returning molecules (Fig 3) In this case the water vapor pressure over the liquid water is called saturated water pressure

                          Saturated water vapor pressure is a function of temperature only and independent on the presence of other gases

                          The temperature dependence is exponential In the case of water vapor the semi empirical dependence reads as

                          DTTCT

                          BA

                          sw ep

                          ln

                          where temperature is in Kelvin and A = 7734 B = -7235 C = - 82 D = 0005711

                          132 Air humidity Amount of water vapor in the air can be expressed by several different ways

                          Specific humidity Mass of water vapor per unit mass of humid air air

                          OH

                          m

                          m 2

                          Absolute humidity Mass of water vapor per unit volume of humid air (kgm3) Relative humidity (RH) Ratio of water vapor pressure pw to the saturated water vapor pressure at that temperature multiplied by 100

                          RH = 100)(

                          Tp

                          ppure

                          ws

                          w (153)

                          Saturation ratio S Ratio

                          S =)( Tp

                          ppure

                          ws

                          w (154)

                          From the last two definitions we see that RH = S100 ie their physical meanings are almost the same Supersaturation S - 1 gt 0

                          For the perfect gas a following (experimental) equation of state p = f (T V n) is true

                          pV= nNAkbT (11) where p is pressure V volume n number of moles NA Avogadro number kb

                          Boltzmann constant and T temperature in Kelvin Since kb NA = R (gas constant) for the amount of gas of one mole (n = 1) the equation of state (11) can be written as

                          pV = RT (12) Using simple kinetic theory of gases and Newtonrsquos laws of motion one can show (see for example Understanding Physics (1998) p 249 or Hinds (1982) pp 15-16) that

                          pV = RT = KE = 3

                          2Nmmol (13)

                          where KE is kinetic energy of the molecules composing the perfect gas mmol mass of

                          molecule N number of molecules and 2 average of square of molecular velocities (see below) The expression (13) means that the kinetic energy KE which is also the internal energy of the perfect gas E is independent on pressure volume or molecular weight and depends only on temperature ie KE = E = E (T)

                          Equations derived for the perfect gas work also in the case of mixture of gases provided that the individual gases (components of the gaseous mixture) and the mixture itself behave perfectly Mathematically this means that are valid both the equations of state for each component of the gaseous mixture i

                          piV = niRT (17) and the equation of state for the mixture itself

                          pV = nRT (18) Daltonrsquos law for a mixture of perfect gases The pressure p exerted by a mixture of the perfect gases is the sum of the partial pressures pi of the gases Mathematically it reads p = sum pi (19)

                          Physical meaning of partial pressure According to the Daltonrsquos law for the perfect gases the pressure p exerted by a gaseous mixture is the sum of the partial pressures pi of the gases In the case of the perfect gases the partial pressure pi is simply the pressure which the gas would exert if it occupied the container alone at the same temperature But in the case of the real gases at moderate pressures the interaction between molecules of different gases makes the total pressure being slightly different (smaller) from the simple sum of the pressures of the gas components if they were alone Therefore for the real gas the partial pressure pi of the gas component i in the gaseous mixture is defined as pi = Xi p (115) where p is the total pressure of the mixture(Compare (115) with (110)) It follows from Eqs (19) and (115) that p = (X1 + X2 + X3 + ) p = p1 + p2 + p3 + = sum pi (116) ie similar for the mixture of the perfect gases the sum of the partial pressures of real gases is also equal to the total pressure of the mixture (But total pressure of the mixture of the perfect gases is not equal to that of the real gases)

                          Kelvin equation

                          ps(r) ps(infin) = exp (2 σwρwRvTr) = exp (ar)r = droplet radius

                          ps(r) = the actual vapour pressure of droplet of radius r

                          ps(infin)= the saturation vapour pressure over bulk water

                          σw = surface tension

                          ρw= water density

                          Rv - the universal gas constant T - temperature

                          ExampleSaturation ratio Critical radius 1 012 μm11 00126 μm2 173 nm

                          What is going on with soluble aerosol particles for example such which are composed of NaCl sea salt ammonium sulfate etc

                          Hygroscopy is the ability of a substance to attract water molecules from the atmosphere through either absorption or adsorption

                          Hygroscopic substances include sugar honey glycerol ethanol methanol sulfuric acid many salts and many other substances

                          Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

                          Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

                          All soluble salts will deliquesce if the air is sufficiently humid

                          141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

                          AA

                          A Xp

                          p or pA = XA pA (160)

                          The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

                          Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

                          The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

                          The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

                          Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

                          Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

                          p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

                          wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

                          Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

                          Koumlhler Curve = Kelvin equation + Raoultrsquos law

                          p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

                          wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

                          The critical radius rc and critical supersaturation Sc are calculated as

                          rc= (3ba)12 and Sc= (4 a3[27 b])12

                          httpenwikipediaorgwikiFileKohler_curvespng

                          Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                          As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                          Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

                          • Slide 1
                          • Slide 2
                          • Slide 3
                          • Slide 4
                          • Slide 5
                          • Slide 6
                          • Slide 7
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                          • Slide 29
                          • Slide 30
                          • Slide 31

                            Saturated water vapor pressure is a function of temperature only and independent on the presence of other gases

                            The temperature dependence is exponential In the case of water vapor the semi empirical dependence reads as

                            DTTCT

                            BA

                            sw ep

                            ln

                            where temperature is in Kelvin and A = 7734 B = -7235 C = - 82 D = 0005711

                            132 Air humidity Amount of water vapor in the air can be expressed by several different ways

                            Specific humidity Mass of water vapor per unit mass of humid air air

                            OH

                            m

                            m 2

                            Absolute humidity Mass of water vapor per unit volume of humid air (kgm3) Relative humidity (RH) Ratio of water vapor pressure pw to the saturated water vapor pressure at that temperature multiplied by 100

                            RH = 100)(

                            Tp

                            ppure

                            ws

                            w (153)

                            Saturation ratio S Ratio

                            S =)( Tp

                            ppure

                            ws

                            w (154)

                            From the last two definitions we see that RH = S100 ie their physical meanings are almost the same Supersaturation S - 1 gt 0

                            For the perfect gas a following (experimental) equation of state p = f (T V n) is true

                            pV= nNAkbT (11) where p is pressure V volume n number of moles NA Avogadro number kb

                            Boltzmann constant and T temperature in Kelvin Since kb NA = R (gas constant) for the amount of gas of one mole (n = 1) the equation of state (11) can be written as

                            pV = RT (12) Using simple kinetic theory of gases and Newtonrsquos laws of motion one can show (see for example Understanding Physics (1998) p 249 or Hinds (1982) pp 15-16) that

                            pV = RT = KE = 3

                            2Nmmol (13)

                            where KE is kinetic energy of the molecules composing the perfect gas mmol mass of

                            molecule N number of molecules and 2 average of square of molecular velocities (see below) The expression (13) means that the kinetic energy KE which is also the internal energy of the perfect gas E is independent on pressure volume or molecular weight and depends only on temperature ie KE = E = E (T)

                            Equations derived for the perfect gas work also in the case of mixture of gases provided that the individual gases (components of the gaseous mixture) and the mixture itself behave perfectly Mathematically this means that are valid both the equations of state for each component of the gaseous mixture i

                            piV = niRT (17) and the equation of state for the mixture itself

                            pV = nRT (18) Daltonrsquos law for a mixture of perfect gases The pressure p exerted by a mixture of the perfect gases is the sum of the partial pressures pi of the gases Mathematically it reads p = sum pi (19)

                            Physical meaning of partial pressure According to the Daltonrsquos law for the perfect gases the pressure p exerted by a gaseous mixture is the sum of the partial pressures pi of the gases In the case of the perfect gases the partial pressure pi is simply the pressure which the gas would exert if it occupied the container alone at the same temperature But in the case of the real gases at moderate pressures the interaction between molecules of different gases makes the total pressure being slightly different (smaller) from the simple sum of the pressures of the gas components if they were alone Therefore for the real gas the partial pressure pi of the gas component i in the gaseous mixture is defined as pi = Xi p (115) where p is the total pressure of the mixture(Compare (115) with (110)) It follows from Eqs (19) and (115) that p = (X1 + X2 + X3 + ) p = p1 + p2 + p3 + = sum pi (116) ie similar for the mixture of the perfect gases the sum of the partial pressures of real gases is also equal to the total pressure of the mixture (But total pressure of the mixture of the perfect gases is not equal to that of the real gases)

                            Kelvin equation

                            ps(r) ps(infin) = exp (2 σwρwRvTr) = exp (ar)r = droplet radius

                            ps(r) = the actual vapour pressure of droplet of radius r

                            ps(infin)= the saturation vapour pressure over bulk water

                            σw = surface tension

                            ρw= water density

                            Rv - the universal gas constant T - temperature

                            ExampleSaturation ratio Critical radius 1 012 μm11 00126 μm2 173 nm

                            What is going on with soluble aerosol particles for example such which are composed of NaCl sea salt ammonium sulfate etc

                            Hygroscopy is the ability of a substance to attract water molecules from the atmosphere through either absorption or adsorption

                            Hygroscopic substances include sugar honey glycerol ethanol methanol sulfuric acid many salts and many other substances

                            Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

                            Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

                            All soluble salts will deliquesce if the air is sufficiently humid

                            141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

                            AA

                            A Xp

                            p or pA = XA pA (160)

                            The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

                            Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

                            The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

                            The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

                            Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

                            Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

                            p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

                            wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

                            Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

                            Koumlhler Curve = Kelvin equation + Raoultrsquos law

                            p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

                            wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

                            The critical radius rc and critical supersaturation Sc are calculated as

                            rc= (3ba)12 and Sc= (4 a3[27 b])12

                            httpenwikipediaorgwikiFileKohler_curvespng

                            Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                            As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                            Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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                              132 Air humidity Amount of water vapor in the air can be expressed by several different ways

                              Specific humidity Mass of water vapor per unit mass of humid air air

                              OH

                              m

                              m 2

                              Absolute humidity Mass of water vapor per unit volume of humid air (kgm3) Relative humidity (RH) Ratio of water vapor pressure pw to the saturated water vapor pressure at that temperature multiplied by 100

                              RH = 100)(

                              Tp

                              ppure

                              ws

                              w (153)

                              Saturation ratio S Ratio

                              S =)( Tp

                              ppure

                              ws

                              w (154)

                              From the last two definitions we see that RH = S100 ie their physical meanings are almost the same Supersaturation S - 1 gt 0

                              For the perfect gas a following (experimental) equation of state p = f (T V n) is true

                              pV= nNAkbT (11) where p is pressure V volume n number of moles NA Avogadro number kb

                              Boltzmann constant and T temperature in Kelvin Since kb NA = R (gas constant) for the amount of gas of one mole (n = 1) the equation of state (11) can be written as

                              pV = RT (12) Using simple kinetic theory of gases and Newtonrsquos laws of motion one can show (see for example Understanding Physics (1998) p 249 or Hinds (1982) pp 15-16) that

                              pV = RT = KE = 3

                              2Nmmol (13)

                              where KE is kinetic energy of the molecules composing the perfect gas mmol mass of

                              molecule N number of molecules and 2 average of square of molecular velocities (see below) The expression (13) means that the kinetic energy KE which is also the internal energy of the perfect gas E is independent on pressure volume or molecular weight and depends only on temperature ie KE = E = E (T)

                              Equations derived for the perfect gas work also in the case of mixture of gases provided that the individual gases (components of the gaseous mixture) and the mixture itself behave perfectly Mathematically this means that are valid both the equations of state for each component of the gaseous mixture i

                              piV = niRT (17) and the equation of state for the mixture itself

                              pV = nRT (18) Daltonrsquos law for a mixture of perfect gases The pressure p exerted by a mixture of the perfect gases is the sum of the partial pressures pi of the gases Mathematically it reads p = sum pi (19)

                              Physical meaning of partial pressure According to the Daltonrsquos law for the perfect gases the pressure p exerted by a gaseous mixture is the sum of the partial pressures pi of the gases In the case of the perfect gases the partial pressure pi is simply the pressure which the gas would exert if it occupied the container alone at the same temperature But in the case of the real gases at moderate pressures the interaction between molecules of different gases makes the total pressure being slightly different (smaller) from the simple sum of the pressures of the gas components if they were alone Therefore for the real gas the partial pressure pi of the gas component i in the gaseous mixture is defined as pi = Xi p (115) where p is the total pressure of the mixture(Compare (115) with (110)) It follows from Eqs (19) and (115) that p = (X1 + X2 + X3 + ) p = p1 + p2 + p3 + = sum pi (116) ie similar for the mixture of the perfect gases the sum of the partial pressures of real gases is also equal to the total pressure of the mixture (But total pressure of the mixture of the perfect gases is not equal to that of the real gases)

                              Kelvin equation

                              ps(r) ps(infin) = exp (2 σwρwRvTr) = exp (ar)r = droplet radius

                              ps(r) = the actual vapour pressure of droplet of radius r

                              ps(infin)= the saturation vapour pressure over bulk water

                              σw = surface tension

                              ρw= water density

                              Rv - the universal gas constant T - temperature

                              ExampleSaturation ratio Critical radius 1 012 μm11 00126 μm2 173 nm

                              What is going on with soluble aerosol particles for example such which are composed of NaCl sea salt ammonium sulfate etc

                              Hygroscopy is the ability of a substance to attract water molecules from the atmosphere through either absorption or adsorption

                              Hygroscopic substances include sugar honey glycerol ethanol methanol sulfuric acid many salts and many other substances

                              Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

                              Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

                              All soluble salts will deliquesce if the air is sufficiently humid

                              141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

                              AA

                              A Xp

                              p or pA = XA pA (160)

                              The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

                              Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

                              The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

                              The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

                              Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

                              Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

                              p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

                              wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

                              Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

                              Koumlhler Curve = Kelvin equation + Raoultrsquos law

                              p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

                              wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

                              The critical radius rc and critical supersaturation Sc are calculated as

                              rc= (3ba)12 and Sc= (4 a3[27 b])12

                              httpenwikipediaorgwikiFileKohler_curvespng

                              Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                              As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                              Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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                                For the perfect gas a following (experimental) equation of state p = f (T V n) is true

                                pV= nNAkbT (11) where p is pressure V volume n number of moles NA Avogadro number kb

                                Boltzmann constant and T temperature in Kelvin Since kb NA = R (gas constant) for the amount of gas of one mole (n = 1) the equation of state (11) can be written as

                                pV = RT (12) Using simple kinetic theory of gases and Newtonrsquos laws of motion one can show (see for example Understanding Physics (1998) p 249 or Hinds (1982) pp 15-16) that

                                pV = RT = KE = 3

                                2Nmmol (13)

                                where KE is kinetic energy of the molecules composing the perfect gas mmol mass of

                                molecule N number of molecules and 2 average of square of molecular velocities (see below) The expression (13) means that the kinetic energy KE which is also the internal energy of the perfect gas E is independent on pressure volume or molecular weight and depends only on temperature ie KE = E = E (T)

                                Equations derived for the perfect gas work also in the case of mixture of gases provided that the individual gases (components of the gaseous mixture) and the mixture itself behave perfectly Mathematically this means that are valid both the equations of state for each component of the gaseous mixture i

                                piV = niRT (17) and the equation of state for the mixture itself

                                pV = nRT (18) Daltonrsquos law for a mixture of perfect gases The pressure p exerted by a mixture of the perfect gases is the sum of the partial pressures pi of the gases Mathematically it reads p = sum pi (19)

                                Physical meaning of partial pressure According to the Daltonrsquos law for the perfect gases the pressure p exerted by a gaseous mixture is the sum of the partial pressures pi of the gases In the case of the perfect gases the partial pressure pi is simply the pressure which the gas would exert if it occupied the container alone at the same temperature But in the case of the real gases at moderate pressures the interaction between molecules of different gases makes the total pressure being slightly different (smaller) from the simple sum of the pressures of the gas components if they were alone Therefore for the real gas the partial pressure pi of the gas component i in the gaseous mixture is defined as pi = Xi p (115) where p is the total pressure of the mixture(Compare (115) with (110)) It follows from Eqs (19) and (115) that p = (X1 + X2 + X3 + ) p = p1 + p2 + p3 + = sum pi (116) ie similar for the mixture of the perfect gases the sum of the partial pressures of real gases is also equal to the total pressure of the mixture (But total pressure of the mixture of the perfect gases is not equal to that of the real gases)

                                Kelvin equation

                                ps(r) ps(infin) = exp (2 σwρwRvTr) = exp (ar)r = droplet radius

                                ps(r) = the actual vapour pressure of droplet of radius r

                                ps(infin)= the saturation vapour pressure over bulk water

                                σw = surface tension

                                ρw= water density

                                Rv - the universal gas constant T - temperature

                                ExampleSaturation ratio Critical radius 1 012 μm11 00126 μm2 173 nm

                                What is going on with soluble aerosol particles for example such which are composed of NaCl sea salt ammonium sulfate etc

                                Hygroscopy is the ability of a substance to attract water molecules from the atmosphere through either absorption or adsorption

                                Hygroscopic substances include sugar honey glycerol ethanol methanol sulfuric acid many salts and many other substances

                                Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

                                Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

                                All soluble salts will deliquesce if the air is sufficiently humid

                                141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

                                AA

                                A Xp

                                p or pA = XA pA (160)

                                The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

                                Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

                                The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

                                The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

                                Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

                                Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

                                p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

                                wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

                                Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

                                Koumlhler Curve = Kelvin equation + Raoultrsquos law

                                p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

                                wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

                                The critical radius rc and critical supersaturation Sc are calculated as

                                rc= (3ba)12 and Sc= (4 a3[27 b])12

                                httpenwikipediaorgwikiFileKohler_curvespng

                                Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                                As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                                Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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                                  Equations derived for the perfect gas work also in the case of mixture of gases provided that the individual gases (components of the gaseous mixture) and the mixture itself behave perfectly Mathematically this means that are valid both the equations of state for each component of the gaseous mixture i

                                  piV = niRT (17) and the equation of state for the mixture itself

                                  pV = nRT (18) Daltonrsquos law for a mixture of perfect gases The pressure p exerted by a mixture of the perfect gases is the sum of the partial pressures pi of the gases Mathematically it reads p = sum pi (19)

                                  Physical meaning of partial pressure According to the Daltonrsquos law for the perfect gases the pressure p exerted by a gaseous mixture is the sum of the partial pressures pi of the gases In the case of the perfect gases the partial pressure pi is simply the pressure which the gas would exert if it occupied the container alone at the same temperature But in the case of the real gases at moderate pressures the interaction between molecules of different gases makes the total pressure being slightly different (smaller) from the simple sum of the pressures of the gas components if they were alone Therefore for the real gas the partial pressure pi of the gas component i in the gaseous mixture is defined as pi = Xi p (115) where p is the total pressure of the mixture(Compare (115) with (110)) It follows from Eqs (19) and (115) that p = (X1 + X2 + X3 + ) p = p1 + p2 + p3 + = sum pi (116) ie similar for the mixture of the perfect gases the sum of the partial pressures of real gases is also equal to the total pressure of the mixture (But total pressure of the mixture of the perfect gases is not equal to that of the real gases)

                                  Kelvin equation

                                  ps(r) ps(infin) = exp (2 σwρwRvTr) = exp (ar)r = droplet radius

                                  ps(r) = the actual vapour pressure of droplet of radius r

                                  ps(infin)= the saturation vapour pressure over bulk water

                                  σw = surface tension

                                  ρw= water density

                                  Rv - the universal gas constant T - temperature

                                  ExampleSaturation ratio Critical radius 1 012 μm11 00126 μm2 173 nm

                                  What is going on with soluble aerosol particles for example such which are composed of NaCl sea salt ammonium sulfate etc

                                  Hygroscopy is the ability of a substance to attract water molecules from the atmosphere through either absorption or adsorption

                                  Hygroscopic substances include sugar honey glycerol ethanol methanol sulfuric acid many salts and many other substances

                                  Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

                                  Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

                                  All soluble salts will deliquesce if the air is sufficiently humid

                                  141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

                                  AA

                                  A Xp

                                  p or pA = XA pA (160)

                                  The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

                                  Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

                                  The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

                                  The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

                                  Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

                                  Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

                                  p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

                                  wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

                                  Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

                                  Koumlhler Curve = Kelvin equation + Raoultrsquos law

                                  p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

                                  wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

                                  The critical radius rc and critical supersaturation Sc are calculated as

                                  rc= (3ba)12 and Sc= (4 a3[27 b])12

                                  httpenwikipediaorgwikiFileKohler_curvespng

                                  Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                                  As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                                  Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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                                    Physical meaning of partial pressure According to the Daltonrsquos law for the perfect gases the pressure p exerted by a gaseous mixture is the sum of the partial pressures pi of the gases In the case of the perfect gases the partial pressure pi is simply the pressure which the gas would exert if it occupied the container alone at the same temperature But in the case of the real gases at moderate pressures the interaction between molecules of different gases makes the total pressure being slightly different (smaller) from the simple sum of the pressures of the gas components if they were alone Therefore for the real gas the partial pressure pi of the gas component i in the gaseous mixture is defined as pi = Xi p (115) where p is the total pressure of the mixture(Compare (115) with (110)) It follows from Eqs (19) and (115) that p = (X1 + X2 + X3 + ) p = p1 + p2 + p3 + = sum pi (116) ie similar for the mixture of the perfect gases the sum of the partial pressures of real gases is also equal to the total pressure of the mixture (But total pressure of the mixture of the perfect gases is not equal to that of the real gases)

                                    Kelvin equation

                                    ps(r) ps(infin) = exp (2 σwρwRvTr) = exp (ar)r = droplet radius

                                    ps(r) = the actual vapour pressure of droplet of radius r

                                    ps(infin)= the saturation vapour pressure over bulk water

                                    σw = surface tension

                                    ρw= water density

                                    Rv - the universal gas constant T - temperature

                                    ExampleSaturation ratio Critical radius 1 012 μm11 00126 μm2 173 nm

                                    What is going on with soluble aerosol particles for example such which are composed of NaCl sea salt ammonium sulfate etc

                                    Hygroscopy is the ability of a substance to attract water molecules from the atmosphere through either absorption or adsorption

                                    Hygroscopic substances include sugar honey glycerol ethanol methanol sulfuric acid many salts and many other substances

                                    Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

                                    Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

                                    All soluble salts will deliquesce if the air is sufficiently humid

                                    141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

                                    AA

                                    A Xp

                                    p or pA = XA pA (160)

                                    The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

                                    Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

                                    The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

                                    The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

                                    Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

                                    Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

                                    p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

                                    wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

                                    Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

                                    Koumlhler Curve = Kelvin equation + Raoultrsquos law

                                    p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

                                    wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

                                    The critical radius rc and critical supersaturation Sc are calculated as

                                    rc= (3ba)12 and Sc= (4 a3[27 b])12

                                    httpenwikipediaorgwikiFileKohler_curvespng

                                    Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                                    As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                                    Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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                                      Kelvin equation

                                      ps(r) ps(infin) = exp (2 σwρwRvTr) = exp (ar)r = droplet radius

                                      ps(r) = the actual vapour pressure of droplet of radius r

                                      ps(infin)= the saturation vapour pressure over bulk water

                                      σw = surface tension

                                      ρw= water density

                                      Rv - the universal gas constant T - temperature

                                      ExampleSaturation ratio Critical radius 1 012 μm11 00126 μm2 173 nm

                                      What is going on with soluble aerosol particles for example such which are composed of NaCl sea salt ammonium sulfate etc

                                      Hygroscopy is the ability of a substance to attract water molecules from the atmosphere through either absorption or adsorption

                                      Hygroscopic substances include sugar honey glycerol ethanol methanol sulfuric acid many salts and many other substances

                                      Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

                                      Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

                                      All soluble salts will deliquesce if the air is sufficiently humid

                                      141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

                                      AA

                                      A Xp

                                      p or pA = XA pA (160)

                                      The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

                                      Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

                                      The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

                                      The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

                                      Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

                                      Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

                                      p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

                                      wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

                                      Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

                                      Koumlhler Curve = Kelvin equation + Raoultrsquos law

                                      p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

                                      wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

                                      The critical radius rc and critical supersaturation Sc are calculated as

                                      rc= (3ba)12 and Sc= (4 a3[27 b])12

                                      httpenwikipediaorgwikiFileKohler_curvespng

                                      Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                                      As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                                      Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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                                        What is going on with soluble aerosol particles for example such which are composed of NaCl sea salt ammonium sulfate etc

                                        Hygroscopy is the ability of a substance to attract water molecules from the atmosphere through either absorption or adsorption

                                        Hygroscopic substances include sugar honey glycerol ethanol methanol sulfuric acid many salts and many other substances

                                        Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

                                        Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

                                        All soluble salts will deliquesce if the air is sufficiently humid

                                        141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

                                        AA

                                        A Xp

                                        p or pA = XA pA (160)

                                        The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

                                        Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

                                        The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

                                        The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

                                        Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

                                        Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

                                        p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

                                        wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

                                        Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

                                        Koumlhler Curve = Kelvin equation + Raoultrsquos law

                                        p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

                                        wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

                                        The critical radius rc and critical supersaturation Sc are calculated as

                                        rc= (3ba)12 and Sc= (4 a3[27 b])12

                                        httpenwikipediaorgwikiFileKohler_curvespng

                                        Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                                        As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                                        Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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                                        • Slide 31

                                          Hygroscopy is the ability of a substance to attract water molecules from the atmosphere through either absorption or adsorption

                                          Hygroscopic substances include sugar honey glycerol ethanol methanol sulfuric acid many salts and many other substances

                                          Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

                                          Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

                                          All soluble salts will deliquesce if the air is sufficiently humid

                                          141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

                                          AA

                                          A Xp

                                          p or pA = XA pA (160)

                                          The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

                                          Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

                                          The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

                                          The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

                                          Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

                                          Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

                                          p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

                                          wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

                                          Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

                                          Koumlhler Curve = Kelvin equation + Raoultrsquos law

                                          p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

                                          wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

                                          The critical radius rc and critical supersaturation Sc are calculated as

                                          rc= (3ba)12 and Sc= (4 a3[27 b])12

                                          httpenwikipediaorgwikiFileKohler_curvespng

                                          Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                                          As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                                          Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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                                            Deliquescent materials (mostly salts) have a strong affinity for water Such materials absorb a large amount of moisture (water vapor) from the atmosphere until it dissolves in the absorbed water and forms an aqueous solution

                                            Deliquescence occurs when the vapour pressure of aqueous solution is smaller than the partial pressure of water in the atmosphere

                                            All soluble salts will deliquesce if the air is sufficiently humid

                                            141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

                                            AA

                                            A Xp

                                            p or pA = XA pA (160)

                                            The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

                                            Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

                                            The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

                                            The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

                                            Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

                                            Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

                                            p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

                                            wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

                                            Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

                                            Koumlhler Curve = Kelvin equation + Raoultrsquos law

                                            p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

                                            wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

                                            The critical radius rc and critical supersaturation Sc are calculated as

                                            rc= (3ba)12 and Sc= (4 a3[27 b])12

                                            httpenwikipediaorgwikiFileKohler_curvespng

                                            Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                                            As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                                            Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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                                              141 Raoultrsquos law a) Ideal solution The expression (158) shows that the chemical potential of the liquid A in the solution increases with increasing the partial vapor pressure pA and becomes equal to the chemical potential of pure liquid when pA = pA The French chemist F Raoult experimentally found that the ratio of the partial vapor pressure of the component A to its vapor pressure as a pure liquid is approximately equal to the mole fraction XA (see 113) in the solution ie

                                              AA

                                              A Xp

                                              p or pA = XA pA (160)

                                              The Eq (160) is known as the Raoultrsquos law The Raoultrsquos law is valid also for the component B Linear dependence of the partial vapor pressures pA and pB are shown by the dashed lines in Fig 6

                                              Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

                                              The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

                                              The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

                                              Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

                                              Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

                                              p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

                                              wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

                                              Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

                                              Koumlhler Curve = Kelvin equation + Raoultrsquos law

                                              p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

                                              wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

                                              The critical radius rc and critical supersaturation Sc are calculated as

                                              rc= (3ba)12 and Sc= (4 a3[27 b])12

                                              httpenwikipediaorgwikiFileKohler_curvespng

                                              Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                                              As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                                              Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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                                                Fig 6 Equilibrium partial pressures of the components of ideal and non-ideal binary solution as a function of the mole fraction XA For the real solution relationships between the pA pB and the mole fractions XA XB are not linear as it is in the case of ideal solution where the linear relationships are shown by the straight dashed lines LR and KQ When XA rarr 1 then we have a dilute solution of B in A In this region the Raoultrsquos law pA = XA pA is applied for the component A For the component B the Henryrsquos law pB = KB XB is applied In the region where XA rarr 0 we have the Raoultrsquos law pB = XB pB for B component and the Henryrsquos law pA = KA XA for A component The straight lines LM and KN depict the Henryrsquos law

                                                The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

                                                The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

                                                Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

                                                Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

                                                p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

                                                wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

                                                Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

                                                Koumlhler Curve = Kelvin equation + Raoultrsquos law

                                                p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

                                                wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

                                                The critical radius rc and critical supersaturation Sc are calculated as

                                                rc= (3ba)12 and Sc= (4 a3[27 b])12

                                                httpenwikipediaorgwikiFileKohler_curvespng

                                                Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                                                As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                                                Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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                                                  The solutions which obey the Raoultrsquos law throughout the whole composition range from pure A to pure B are called ideal solutions

                                                  The solutions which components are structurally similar obey the Raoultrsquos law very well In Fig 6 the equilibrium partial pressures of the components A and B in the ideal solution are shown by dashed lines of LR and KQ Solution is only ideal if is satisfied for each component

                                                  Dissimilar liquids (large difference in the liquid structures) significantly depart from the Raoultrsquos law Nevertheless even for these mixtures the Raoultrsquos law is obeyed closely for the component in excess as it approaches purity ie when XA rarr 1 or XA rarr 0 (Fig 6)

                                                  Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

                                                  p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

                                                  wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

                                                  Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

                                                  Koumlhler Curve = Kelvin equation + Raoultrsquos law

                                                  p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

                                                  wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

                                                  The critical radius rc and critical supersaturation Sc are calculated as

                                                  rc= (3ba)12 and Sc= (4 a3[27 b])12

                                                  httpenwikipediaorgwikiFileKohler_curvespng

                                                  Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                                                  As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                                                  Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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                                                    Raoultrsquos law Mathematically for a plane water surface the reduction in vapour pressure due to the presence of a non-volatile solute is expressed

                                                    p (infin)ps(infin) = 1 ndash (3νmsMw)(4 πMsρwr3) = 1 - br3

                                                    wherep (infin) - the saturation vapour pressure of pure water ps (infin) - the saturation vapour pressure of bulk solution Ms- molecular weight of the solute Ms- mass of the solute Ν- degree of dissociation

                                                    Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

                                                    Koumlhler Curve = Kelvin equation + Raoultrsquos law

                                                    p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

                                                    wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

                                                    The critical radius rc and critical supersaturation Sc are calculated as

                                                    rc= (3ba)12 and Sc= (4 a3[27 b])12

                                                    httpenwikipediaorgwikiFileKohler_curvespng

                                                    Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                                                    As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                                                    Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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                                                      Combining the Kelvin equation and the expression from the Raoultrsquos law we can obtain so called Kohler equation

                                                      Koumlhler Curve = Kelvin equation + Raoultrsquos law

                                                      p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

                                                      wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

                                                      The critical radius rc and critical supersaturation Sc are calculated as

                                                      rc= (3ba)12 and Sc= (4 a3[27 b])12

                                                      httpenwikipediaorgwikiFileKohler_curvespng

                                                      Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                                                      As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                                                      Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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                                                        Koumlhler Curve = Kelvin equation + Raoultrsquos law

                                                        p(r)ps(infin) = (1 - br3)middotexp(ar) asymp 1 + ar - br3

                                                        wherea ~ 33 10-7T [m]b ~ 43 10-6i Msms [m3mol]Ms= molecular mass of salt [kgmol]ms= mass of salt [kg]

                                                        The critical radius rc and critical supersaturation Sc are calculated as

                                                        rc= (3ba)12 and Sc= (4 a3[27 b])12

                                                        httpenwikipediaorgwikiFileKohler_curvespng

                                                        Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                                                        As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                                                        Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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                                                          httpenwikipediaorgwikiFileKohler_curvespng

                                                          Kohler curves show how the critical diameter and criticalsupersaturation are dependent upon the amount of solute

                                                          As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                                                          Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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                                                            As humidity increases aerosol continues to swell even after vapor saturation is reached Once a critical supersaturation is reached corresponding to the peak of the Koumlhler curve for that particle a particle becomes activated as a cloud droplet Activated particles are no longer in stable equilibrium with the vapor phase but are able to continue to grow by vapor deposition provided that conditions remain supersaturated

                                                            Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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                                                              Droplet size is determined by the number of particles activated and the amount of water vapor available for condensation which is generally determined by the vertical height of an adiabatic ascent If droplets are able to grow to a sufficient size and the cloud exists for a sufficient length of time droplets will coalesce as they collide with each other through random motion gravitational settling or motion within the dynamics of the cloud system

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