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Bernoulli's Eqn

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    Bernoulli equation

    Daniel Bernoulli (1710-1782)

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    Bernoulli: preamble

    Want to discuss the properties of a moving fluid.

    Will do this initially under the simplest possible

    conditions, leading to Bernoulli’s equation. The

    following restrictions apply.

    •  Flow is inviscid, there are no viscous drag forces•  Heat conduction is not possible for an inviscid

    flow

    •  The fluid is incompressible .

    • The flow is steady (velocity pattern constant).

    •  The paths traveled by small sections of the fluidare well defined.

    •  Will be implicitly using the Euler equations of 

    motion (discussed later)

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    Coordinates and streamlines

    • Each piece of fluid has velocity  v   .

    •  Steady flow, nothing changes with time at givenlocation. All particles passing through (1)   end

    up at (2)   with velocity  v

    • The trajectories followed by the particles are

    called streamlines.

    •  Describe motion is terms of distanced traveledalong streamline,  s  .

    •  Velocity given by

     |v|

    =   dsdt

      . Normal to velocity

    is  n̂  .

    •   Stream-line can bend,  R   is radius of curvature.

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    Coordinates and streamlines

    Using body fixed coordinates. If the particles change

    speed along stream-line, or if stream-line bends, then

    accelerations must be present.

    The tangential acceleration

    as =  dvdt

      =  ∂v∂s

    dsdt

      = v ∂v∂s

    The normal acceleration

    an  = v2

    R

    The radius of curvature  R   changes along the

    streamline.

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    Streamline coordinates

    It is convenient to use a coordinate system defined in

    terms of the flow streamlines. The coordinate along

    the streamline is  s   and the coordinate normal to the

    streamline is  n   . The unit vectors for the streamlinecoordinates are  ŝ   and n̂  .

    The direction of   ŝ  will be chosen to be in the same

    direction as the velocity. So  v = vŝ  .

    s

    n^

    s^

    V

    s = 0

    s = s1

    s = s2

    n = n2

    n = n1

    n = 0

    Streamlines

     y

     x 

    The flow plane is covered with an orthogonal curvednet of coordinate lines and  v = v(s, n)ŝ   and

    ŝ = ŝ(s, n)   for steady flow.

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    Forces on streamlines

    Any particle travelling along the streamline will be

    subjected to a number of forces.

    The relevant Forces for Bernoulli’s equation are

    gravity and pressure.

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    Streamlines   F    = ma

    Will resolve forces in directions parallel   ŝ   and

    perpendicular n̂   to particles motions.   y   is out of 

    page,  z   is down,  x   is horizontal.

    δF s   =   δm as = δm v ∂v∂s

    =   ρδV v∂v

    ∂s

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    Streamlines   F    = ma

    Resolve forces

    δW s = δW   sin θ = γδV   sin θ

    δW s   would be zero for horizontal motion.

    The pressure changes with height. Let  p   be pressure

    in middle of fluid slab. Let  p + δps   be pressure in

    front of slab and  p− δps   be pressure behind slab.From Taylors series

    δps = ∂p

    ∂s

    δs

    2

    The net pressure force

    δF  ps   = ( p−

    δps)δnδy−

    ( p + δps)δnδy

    =   −2δpsδnδy  = −∂p∂s

    δsδnδy = −∂p∂s

    δV 

    Net force

    δF s   =   δW s + δF  ps

    =

    −γ  sin θ −  ∂p

    ∂s

    δV 

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    Bernoulli equation

    Equate two expressions for  δF s

    δF s =−γ  sin θ −  ∂p∂s δV    =   ρδV v ∂v∂s⇒−γ  sin θ −  ∂p

    ∂s

      =   ρ v

    ∂v

    ∂s

    The change in in fluid particle speed along a

    streamline is accomplished by a combination of pressure and gravity forces.

    •   Now use sin θ =   dzds

    •  And  v dv

    ds  =   1

    2

    dv2

    ds

    •   And  dp =   ∂p∂s

    ds +   ∂p∂n

    dn

    •   Along streamline  dn = 0

    −γ 

    dz

    ds − dp

    ds  =

      1

    dv2

    ds

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    Bernoulli, compact expression

    Now making the assumption that density is constant,

    Bernoulli’s equation is obtained

    γ dz

    ds +

     dp

    ds +

     1

    dv2

    ds  = 0

    d

    ds

    γz + p +

     1

    2ρv2

      = 0

    γz + p + 12

    ρv2 = Constant

    The constant density assumption (incompressible

    flow) is good for liquids (sometimes gases at low

    speed). Bernoulli’s equation presented in 1738

    monograph  Hydrodynamics  by Daniel Bernoulli.

    If one has compressible fluid

       dp

    ρ  +

     1

    2v2 + gz   = Constant

    and knowledge of how  ρ   varies with  p  .

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    Forces normal to streamline

    The acceleration normal to the streamline is  an =  v2

    R

    where  R   is the local radius of curvature of the

    streamline.

    δF n   =   (δm)v

    2

    R  =   ρ δV v

    2

    R

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    Forces normal to streamline

    A change in stream direction occurs from pressure

    and/or and gravity forces. Resolve forces

    δW n  = δW   cos θ = γδV  cos θ

    δW n   would be zero for vertical motion.

    The pressure changes with height. Let  p   be pressure

    in middle of fluid slab,  p + δpn   is pressure at top of slab and  p− δpn   be pressure at bottom of slab.From Taylors series

    δpn =  ∂p

    ∂n

    δn

    2

    The net pressure force,  δF  pn

    δF  pn   = ( p− δpn)δs δy − ( p + δpn)δs δy=   −2δpnδn δy = −∂p

    ∂nδn δs δy  = − ∂p

    ∂nδV 

    Need to combine pressure and weight forces to get

    net Force

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    Forces normal to streamline

    Combine weight and pressure forces

    δF n   =   δW n + δF  pn

    =

    −γ  cos θ −  ∂p

    ∂n

    δV   =

      ρδV v2

    R

    Pressure and weight forces imbalance produces the

    curvature. For gas flows it is common to use

    ∂p

    ∂n = −ρv

    2

    R

    The pressures increases

    with distance away fromthe center of curvature

    ( ∂p∂n

      is negative since

    ρv2/R   is positive).

    For straight parallel streamlines (in gases),   ∂p∂n  = 0 .

    No pressure change across streamlines

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    Forces normal to streamline

    Will consider fluid parameters normal to stream line

    γ  cos θ +

     ∂p

    ∂n+

     ρv2

    R  = 0

    •   ∂p∂n

     =   dpdn

      since  s   is constant.

    •   cos θ =   dzdn

    and so for incompressible flows

    dp

    dn + γ 

    dz

    dn +

     ρv2

    R  = 0

    dp

    dn + γ 

    dz

    dn +

     ρv2

    R  = 0

    ddn

     ( p + γz) +  ρv2

    R  = 0

     p + γz + ρ

       v2

    Rdn = Constant

    For a compressible substance, the best reduction is   dp

    ρ  +

       v2

    R  + gz  = Constant

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    Interpretation for incompressible flows

    Along the streamline

    γz + p + 12 ρv2 = Constant

    Across the streamline

     p + γz + ρ

       v2

    Rdn = Constant

    The units of Bernoulli’s equations are J m−3 . This

    is not surprising since both equations arose from an

    integration of the equation of motion for the force

    along the  s   and  n   directions.

    The Bernoulli equation along the stream-line is a

    statement of the work energy theorem. As the

    particle moves, the pressure and gravitational forces

    can do work, resulting in a change in the kineticenergy.

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    Dynamic and static pressures

     p + 12

    ρv2 + ρgz = constant

    Static pressure is the pressure as measured moving

    with the fluid. (e.g. static with fluid). This is the  p

    term in Bernoulli’s equation. Imagine moving along

    the fluid with a pressure gauge.

    Some times the  ρgz   term in Bernoulli’s equation is

    called the hydrostatic pressure. (e.g. it is the change

    in pressure due to change in elevation.)

    Dynamic pressure is a pressure that occurs when

    kinetic energy of the flowing fluid is converted into

    pressure rise. This is the pressure associated with

    the  1

    2ρv2

    term in Bernoulli’s equation.

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    Dynamic and static pressures

    The static pressure at 1   can be estimated by the

    height of the column.

     p1   =   γh3−1 + p3

    =   γh3−1 + γh4−3

    =   γh

    (1)   (2)

    (3)

    (4)

    h3-1

    h h4-3

    ρ 

    Open

     H 

    V 1 = V V 2 = 0

    The dynamic pressure at 2   is estimated by

     p2   =   p1 + 1

    2ρv21

    The additional pressure due to the dynamic pressure

    will cause the fluid to rise a height of  H > h  .

    The point (2)   is called a stagnation point.

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    The stagnation point

    Stagnation point

    (a)

    Stagnation streamline

    Stagnation point

    (b)

    When fluid flows around any stationary body, some

    of the streamlines pass over and some pass under the

    object. But there is always a stagnation point where

    the stagnation streamline terminates. The

    stagnation pressure is

     pstagnation   =   p + 1

    2ρv2

    v   is velocity at some point on stream-line away from

    obstruction.

    The total pressure,  pT 

     pT    =   p + 12 ρv2 + γz

    is sum of static, dynamic and hydrostatic pressures.

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    The pitot tube

    Knowledge of static and stagnation pressures makes

    it possible to determine the fluid velocity. Geometry

    arranged so that elevation differences have little

    impact. The free stream pressure is  p  .

    Stagnation pressure

     p2 = p3 = p +

     1

    2 ρv2

     p

    (1)

    (2)

    (4)

    (3)

    Static pressure is just  p1 = p ≈  p4   . Combiningequations

     p   =   p4 = p3 −  12

    ρv2

    Rearranging leads to

    v = 

     p3 − p4ρ

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    The pitot tube: complications

    The main question is de-sign of pitot tubes is where

    to place the orifice to mea-

    sure the static pressure.

    American Blower company

    National Physical laboratory (England)

    American Society of Heating & Ventilating Engineers

    The static pressure doesvary along the length of 

    the tube. More com-

    plicated analysis than

    Bernoulli required here.

    Also make mouth of tube smooth.

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    The free jet

    The free jet result was first obtained in 1643 by

    Evangelista Torricelli.

     p1 + 1

    2ρv21 + γz1   =   p2 +

     1

    2ρv22 + γz2

    γz1   =  1

    2ρv22

    •   p1 = patm = 0 ; gauge pressure•   v1 ≈ 0 ; large surface, so  v1 

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    The free jet

    γz1   =  1

    2ρv22

    v2   =

     2γh

    ρ  =

     2gh

    Outside nozzle, stream continues to fall and at  (5)

    v2   = =  2g(h + H )Result  v  = √ 2gh   is speed of freely falling bodystarting from rest.

    For the fluid, all the potential energy is converted to

    kinetic energy when jet leaves tank. (assume no

    viscous forces).

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    Free jet, fine details

    Horizontal nozzle, veloc-

    ity at center line   v2   is

    slightly smaller than   v3

    and slightly larger than

    v1   .

    For   d    h   , OK to usev2   as average velocity.

    Streamlines cannot follow sharp corner exactly.

    Would take an infinite pressure gradient to achieve

    zero radius of curvature

    (i.e.   R = 0 ). Uniform velocity only occurs at a-a   line.

    Vena Contracta effect.

    Jet diameter,   d j   is

    slightly smaller than

    hole diameter  dh   .

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    Free jet, Vena contracta effect

    The contraction coefficient,  C d  = A j/Ah   is the ratio

    of the jet area  A j   , and hole area  Ah   .

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    Flow rates

    How much water flows down a channel or through a

    pipe?

    The volume flow rate,

    Q1  is defined as the vol-

    ume of fluid that flowspast an imaginary (or

    real) interface.

    •  Volume of fluid leaving  δV   = v1δtA1•   Rate of volume change   δV  

    δt  = v1A1

    •  The volume flow rate  Q = v1A1•  Mass of fluid leaving  δm = ρv1δtA1

    •   Rate fluid leaving  ṁ =   dmdt   = ρv1A1

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    Equation of continuity

    For a steady state situation, the mass of fluid going

    into the tank must be the same as the mass of fluid

    leaving the tank.

    Mass of water in = Mass of water out

    ρ1A1v1   =   ρ2A2v2

    This is the continuity equation and forincompressible flow

    A1v1   =   A2v2   or   Q1 = Q2

    The equation of continuity and the Bernoulli’s

    equation are used into conjunction to analyze many

    flow situations.

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    Flow rate: Example 1

    Given the water velocity

    at   (2)   is   8.0 m/s   and

    the pipe diameter is 0.10

    m  , what are the volume

    and mass flow rates?

    Q   =   vA = vπ(d/2)2

    = 8.0× π0.0502 = 0.06283 m3/s

    The mass flow is just  Q× ρ   sodm

    dt  = 1000× 0.06283 = 62.83 kg/s

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    Flow rate: Example 2

    A stream of water of wa-

    ter   d   = 0.10 m   flows

    steadily from a tank of diameter   D   = 1.0   m

    as shown in the figure.

    What flow-rate is needed

    from the inlet to maintain

    a constant water volumein the header tank depth?

    The depth of water at the

    outlet is 2.0 m   .

    Can regard outlet as a free jet (note water level at

    (1)   is not going down).

    v2   = 

    2gh  =√ 

    2× 9.8× 2.0 = 6.26 m/s⇒ Q2   =   A2v2 = π(0.050)26.26 = 0.0492 m3/s

    =   Q1

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    Flow rate measurement

    One way to measure flow-rate is to place a

    constriction in a pipe. The resulting change in

    velocity (continuity equation), leads to a pressure

    difference. The absolute fluid velocity can bedetermined from pressure difference between (1)   and

    (2) .

    The Orifice, Nozzle and Venturi meters analysis here

    ignores viscous, compressibility and other real-world

    effects.

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    Flow rate measurement: 2

    Want to determine flow rate, need  v2

    v1A1   =   v2A2

    ⇒ v1   =   A2A1

    v2

     p2 + 1

    2ρv22   =   p1 +

     1

    2ρv21

    ⇒  12

    ρv22 − 1

    2ρv21   =   p2 − p1

    ⇒  12

    ρv22 − 1

    A22

    A21

    v22   =   p2 − p1

    ⇒ v2

    2   =

      2( p2−

     p1)

    ρ

    1−  A22A21

    So the flow rate is

    Q   =   A2 2( p2 − p1)

    ρ

    1− A2

    2

    A21

    The pressure differences give the flow rate. Real

    world flows are 1%   to 40%   smaller.

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    Bernoulli and Cavitation

    The temperature at which water boils depends on

    pressure.

    T   (oC)   pvap  (kPa)

    10 1.23

    20 2.34

    30 4.24

    40 7.34

    Q

     p

    (Absolute

    pressure)

    (1)  (2)   (3)

    Small Q

    Moderate Q

    Large Q   Incipient cavitation

     pv

    0  x 

    The process of cavitation involves

    •  Fluid velocity increases•   Pressure reduction•   If  p < pvap   , water boils

    •  Bubbles collapse when reach high pressure partof fluid

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    Bernoulli and Cavitation

    Pressure transients exceeding 100 MPa   can be

    produced. These transients can produce structural

    damage to surfaces.

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    Sluice gate flow rate

    The height of water in the channel can be used to

    determine the flow rate of water out the reservoir.

    Q   =   z2b

     2g(z1 − z2)1−   z22

    z21

    ≈ z2b 

    2gz1

    (b)   is the width of the reservoir.

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    Venturi meter problem

    Determine flow

    rate as a function

    of the diameter of the tube.

    0.2 m

    Q

    0.1 m   D

    Use venturi meter equation

    Q   =   A2  2( p2 − p1)

    ρ

    1−  A22A21

    •   A2 = πD2/4 m2

    •   p2− p1 = −γ × 0.20 = −9800× 0.20 = −1960 Pa•   ρ = 1000 kgm−3

    •   1−A22

    /A21

     = 1−D2/0.102 = 1− 100D2 m2

    Q   =   πD2

    4

        −39201000(1− 100D2)  = πD

    2

       0.245

    (100D2 − 1)

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    Sharp crested weir

    •  Between (1)   and (2)   pressure and gravitational

    forces cause fluid to accelerate from  v1 → v2   .•   p1 = γh   and  p2 ≈ 0   forces cause fluid to

    accelerate from  v1 → v2   .

    • Assume flow is like free jet. Average velocity

    across weir is  C 1√ 2gH   ,  C 1   = constant.

    •   Flow rate is

    Q = (Hb)× C  2gH  = C 1b 2gH 3

    The parameter  C 1   is determined empirically.

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    The energy line and hydraulic grade line

    Consider Bernoulli equation divided by  γ  = ρg

     p

    γ  +

     1

    2

    v2

    g  + z   =   H  = Constant on streamline

    The dimensions of the equation are in length. There

    is the pressure head, velocity head, and elevation

    head. The sum,  H    is called the total head.

    The energy line gives the total head available to a

    fluid. It can be measured by measuring thestagnation pressure with a pitot tube.

    The Hydraulic grade line is the line produced from

    the pressure and elevation heads. It is measured with

    a static pitot tube.

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    The energy line and hydraulic grade line

    •  The energy line will be horizontal along thestream line as long as Bernoulli assumptions are

    valid.

    •  The hydraulic grade line will not be horizontal if the fluid velocity changes along the stream line.

    • If forces are present (this does occur in pipe

    flows), then there will be a loss in energy and

    the energy line will not be constant.

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    Example: EL and HGL

    A scale drawing can be used to depict the pressure in

    the tank/pipe system.

    •  The energy line is horizontal

    •   The elevation head at (2)   is converted intoincreased pressure head  p2/γ    and velocity headv22

    /(2g) . The HGL decreases.

    •   At (3) , pressure is atmospheric. So the HGL tothe level of the pipe and the elevation head has

    been converted entirely into a velocity head

    v23

    /(2g) .

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    EL and HGL

    The EL and HGL can depict whether there ispositive pressure  p > patm   or negative pressure

     p < patm   .

    • The water velocity will be constant in curved

    pipe (equation of continuity).

    •  The pressure head will increase or decrease asthe elevation head changes. Useful to know for

    leaking pipes.

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    Limitations on Bernoulli equation

    A number of problems can invalidate the use of the

    Bernoulli equation, these are   compressibility effects ,

    rotational effects ,  unsteady effects .

    Compressibility effects

    When can compressibility effects impact on gas

    flows? Consider stagnation point

    •  Stagnation pressure is greater than staticpressure by   1

    2ρv2 (dynamic pressure), provided

    ρ   constant.

    •  ρ   will not changes too much as long as dynamic

    pressure is not too large when compared to

    static pressure.

    •  So flows at low  v   will be incompressible

    •  But dynamic pressure increases as  v2

    , socompressibility effects most likely at high speed.

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    Compressibility effects

    The isothermal model for an ideal gas,  p = ρR∗T 

    C    =

       dp

    ρ  +

     1

    2v21 + gz1

    C    =   RT  

      dp p

      + 12

    v21 + gz1

    C    =   RT  ln p1 + 1

    2v21 + gz1

    This can be used to get

    v21

    2g + z1 +

     RT 

    g  ln( p1/p2) =

      v22

    2g + z2

    Now write as  p1/p2 = 1 + ( p1 − p2)/p2 = 1 + ∆ p/p2and use ln(1 + x) = x   for  x

    1 .

    v21

    2g + z1 +

     RT 

    g  ln(1 + ∆ p/p2) =

      v22

    2g + z2

    v21

    2g + z1 +

     RT 

    g  (∆ p/p2)   ≈   v

    22

    2g + z2

    This can be reduced to the standard Bernoulliequation. Bernoulli recovered as long as pressure

    differences are not large.

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    Compressibility effects: Isentropic flow

    This is the situation that applies when there is no

    heat transfer or friction during the flow (reasonable

    for many gases). This gas law is  p = ρkD   where  k

    depends on specific heat capacities. Introduce the

    Mach number, Ma = v/c   (ratio of the flow speed to

    the speed of sound). Consideration of the pressure

    ratio between free stream and stagnation points

    leads to p2 − p1

     p1=

      kMa212

      incompressible

     p2 − p1 p1

    =

    1 +

     k − 1Ma21

    +  k

    k−1

    − 1

      compressible

    The compressible and

    incompressible expres-

    sions agree to   2%   for

    Ma 

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    Unsteady effects

    Implicit in the discussion was an assumption that

    the fluid flows along steady state streamlines, so

    v = v(s)   is a function of position along the stream

    and does not contain any explicit time dependence.

    If  v  = v(s, t)   then then it would be necessary to

    include this when integrating along the streamline.

     p1 + 1

    2ρv21 + γz1 = p2 +

     1

    2ρv22 + γz2 + ρ

       t2t1

    ∂p

    ∂sds

    The additional term does complicate matters and

    can only be easily handled under restricted

    circumstances. There are  quasi-steady  flows where

    some time dependence exists, but Bernoulli’s

    equations could be applied as if the flow were steady

    (e.g. the draining of a tank).

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    Rotational effects

    Model of wake behind insect

    Y. D. Afanasyev, Memorial University of 

    Newfoundland

    Bernoulli equation describes motion of fluid particles

    along streamline. If particles  spin  about the

    streamline then Bernoulli is no longer valid.

    Need to characterize   irrotational  and  rotational  flows.