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Stratospheric Chemistry Stratospheric Chemistry EPS 133 28 March – 04 April 2011 EPS 133 28 March – 04 April 2011 Polar Stratospheric Clouds
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Stratospheric Chemistry EPS 133 28 March – 04 April 2011

Dec 31, 2015

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Stratospheric Chemistry EPS 133 28 March – 04 April 2011. Polar Stratospheric Clouds. ATMOSPHERIC ATTENUATION OF SOLAR RADIATION. Solar UV radiation reaching the top of the atmosphere is absorbed by ozone. Based on ozonesonde observations in the 1970s. THE NATURAL OZONE LAYER. - PowerPoint PPT Presentation
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Page 1: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

Stratospheric ChemistryStratospheric ChemistryEPS 133 28 March – 04 April 2011EPS 133 28 March – 04 April 2011

Polar Stratospheric Clouds

Page 2: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

ATMOSPHERIC ATTENUATION OF SOLAR RADIATIONATMOSPHERIC ATTENUATION OF SOLAR RADIATION

Solar UV radiation reaching the top of the atmosphere is absorbed by ozone

Page 3: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

THE NATURAL OZONE LAYERTHE NATURAL OZONE LAYERBased on ozonesonde observations in the 1970s

Page 4: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

1 Dobson Unit (DU) is defined to be 0.01 mm thickness at stp; the ozone layer over Labrador is ~300 DU.

Mean ratio, column O3: air = 5 x 10-7

Page 5: Stratospheric Chemistry EPS 133 28 March – 04 April 2011
Page 6: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

Ozone mixing ratio in parts per million

Page 7: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

SOLAR SPECTRUM AND ABSORPTION X-SECTIONSSOLAR SPECTRUM AND ABSORPTION X-SECTIONS

O2+hv O3+hv

Page 8: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)(1930)

2

2 3

3 2

3 2

(R1) O O + O ( < 240 nm)

(R2) O + O M O M

(R3) O O O ( 320 nm)

(R4) O O 2O

h

h

O O3O2

slow

slow

fast

Odd oxygen family [Ox] = [O3] + [O]

R2

R3

R4

R1

Page 9: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

STEADY-STATE ANALYSIS OF CHAPMAN MECHANISMSTEADY-STATE ANALYSIS OF CHAPMAN MECHANISMLifetime of O atoms:

O 22 2 4 3 2 O2

[O] 11 s

[O][O ][M]+ [O ][O] ak k k C n

…is sufficiently short to assume steady state for O:

3 O2 2 3 3 2

3 2 2 3

x 3

[O]2 3 [O][O ][M]= [O ] 1

[O ]

[O ] [O ]O a O

kR R k k

k C n

…so the budget of O3 is controlled by the budget of Ox.

Lifetime of Ox:

xOx

4 3 4

[O ] 1

2 [O ][O] 2 [O]k k

Steady state for Ox:1

321 2 2

3 O23

1 2 44

3 [O2 1 2 4 [O ] [O O] ]][ aR R kk k

C nk k

k

τOx

Page 10: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

PHOTOLYSIS RATE CONSTANTS: VERTICAL DEPENDENCEPHOTOLYSIS RATE CONSTANTS: VERTICAL DEPENDENCE

0X+ ... ( ) ( )X Xh k q I d

quantumyield

absorptionX-section

photonflux

2 2 3 3optical depth ( ( ) ( ))O O O Od n z n z dz

( )I z dz

( )I z

2 2 3 3

( ) ( ) e

( ( ') ( ')) 'O O O Oz

I z I

n z n z dz

Page 11: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

CHAPMAN MECHANISM vs. OBSERVATIONCHAPMAN MECHANISM vs. OBSERVATION

-3

shapedeterminedby k1nO2

Chapman mechanism reproduces shape, but is too high by factor 2-3missing sink!

Page 12: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

RADICAL REACTION CHAINS IN THE ATMOSPHERERADICAL REACTION CHAINS IN THE ATMOSPHERE

non-radical radical + radicalInitiation:photolysisthermolysisoxidation by O(1D)

radical + non-radical non-radical + radicalPropagation: bimolecularredox reactions

non-radical + non-radicalTermination: radical redox reaction

radical + radical

non-radical + M radical + radical + M 3-body recombination

Page 13: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

WATER VAPOR IN STRATOSPHEREWATER VAPOR IN STRATOSPHERE

Source: transport from troposphere, oxidation of methane (CH4)

                             

H2O mixing ratio

Page 14: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

Initiation:1

2H O + O( ) 2OHD

Propagation: 3 2 2

2 3

3

2

2

OH + O HO O

HO +

Net:

O OH +

2O

2O

3O

Termination:2 2 2OH + HO H O + O

OH HO2H2Oslow

slow

fast HOx radical family

Ozone loss catalyzed by hydrogen oxide Ozone loss catalyzed by hydrogen oxide (HO(HOxx ≡ H + OH + HO ≡ H + OH + HO22) radicals) radicals

Page 15: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

Rate limiting step: Example

OH + O3 -> HO2+ + O2 k1

HO2 + O3 -> OH + O2 k2

HO2 + NO ->->-> OH + NO + O3 k3

{ + O2 + h … }

d[OH] / dt = -d[HO2] / dt = - k1[OH][O3] + k2[O3][HO2] + k3*[NO][HO2] ≈ 0 A

d[O3] / dt = -k1[OH][O3] – k2[HO2][O3] + k3*[NO][HO2] B

To B, add (-1)xA ≈ 0

d[O3] / dt = - 2 k2 [HO2][O3]

Rate limiting step for removal of ozone by Reactions 1, 2, 3

OH + O3

HO2 + O3

HO2 + NO

Page 16: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

STRATOSPHERIC OZONE BUDGET FOR MIDLATITUDES STRATOSPHERIC OZONE BUDGET FOR MIDLATITUDES CONSTRAINED FROM 1980s SPACE SHUTTLE OBSERVATIONSCONSTRAINED FROM 1980s SPACE SHUTTLE OBSERVATIONS

Page 17: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

NITROUS OXIDE IN THE STRATOSPHERENITROUS OXIDE IN THE STRATOSPHERE

                             

H2O mixing ratio

Page 18: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

ATMOSPHERIC CYCLING OF NOATMOSPHERIC CYCLING OF NOxx AND NO AND NOyy

Page 19: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

Rate limiting step, NOx: Example

NO + O3 -> NO2+ + O2 k1

NO2 + hν -> NO + O -> O3 k2

NO2 + O -> NO + O2 k3

d[NO] / dt = -d[NO2] / dt = - k1[NO][O3] + k2[NO2] + k3[NO2][O] ≈ 0 A

d[O3] / dt = -k1[NO][O3] + k2[NO2] - k3[NO2][O] B

To B, add (-1)xA ≈ 0

d[O3] / dt = - 2 k3 [NO2][O]

Rate limiting step for removal of ozone by Reactions 1, 2, 3

NO + O3

NO2 + ONO2 + hv

Page 20: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

STRATOSPHERIC DISTRIBUTION OF CFSTRATOSPHERIC DISTRIBUTION OF CF22ClCl22 (CFC-12) (CFC-12)

Page 21: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

ATMOSPHERIC CYCLING OF ClOATMOSPHERIC CYCLING OF ClOxx AND Cl AND Clyy

Page 22: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

SOURCE GAS CONTRIBUTIONS TOSOURCE GAS CONTRIBUTIONS TOSTRATOSPHERIC CHLORINE (2004)STRATOSPHERIC CHLORINE (2004)

Page 23: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

CHLORINE PARTITIONING IN STRATOSPHERECHLORINE PARTITIONING IN STRATOSPHERE

Page 24: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

WHAT IS A RATE-LIMITING STEP?WHAT IS A RATE-LIMITING STEP?

• From IUPAC: “A rate-controlling (rate-determining or rate-limiting) step in a reaction occurring by a composite reaction sequence is an elementary reaction the rate constant for which exerts a strong effect — stronger than that of any other rate constant — on the overall rate.”

Page 25: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

Latitude Latitude

alti

tud

e

http://ccmc.gsfc.nasa.gov/modelweb/atmos/msise.html

ftp://hanna.ccmc.gsfc.nasa.gov/pub/modelweb/atmospheric/msis/msise90/

Page 26: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

Latitude Latitude

alti

tud

e

Page 27: Stratospheric Chemistry EPS 133 28 March – 04 April 2011
Page 28: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

Prof. James R. Holton

Stratospheric Circulation

Page 29: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

OZONE TREND AT HALLEY BAY, ANTARCTICA (OCTOBER)OZONE TREND AT HALLEY BAY, ANTARCTICA (OCTOBER)

Farman et al. paper published in Nature

1 Dobson Unit (DU) = 0.01 mm O3 STP = 2.69x1016 molecules cm-2

Page 30: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

SPATIAL EXTENT OF THE OZONE HOLESPATIAL EXTENT OF THE OZONE HOLE

Isolated concentric region around Antarctic continent is called the polar vortex.Strong westerly winds, little meridional transport

Mean Octoberdata

Page 31: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

THE POLAR VORTEX (Sep-Oct 2006)THE POLAR VORTEX (Sep-Oct 2006)

Page 32: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

THE OZONE HOLE IS A SPRINGTIME PHENOMENONTHE OZONE HOLE IS A SPRINGTIME PHENOMENON

Page 33: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

VERTICAL STRUCTURE OF THE OZONE HOLE:VERTICAL STRUCTURE OF THE OZONE HOLE:near-total depletion in lower stratospherenear-total depletion in lower stratosphere

Argentine Antarctic station southern tip of S. America

Page 34: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

Sep. 2, 1987

Sep. 16

20 km altitude

ASSOCIATION OF ANTARCTIC OZONE HOLEASSOCIATION OF ANTARCTIC OZONE HOLEWITH HIGH LEVELS OF CLOWITH HIGH LEVELS OF CLO

Sept. 1987 ER-2 aircraft measurements at 20 km altitude south of Punta Arenas

ClO

ClO

O3

O3

Edge ofPolar vortex

Measurements by Jim Anderson’s group (Harvard)

Page 35: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

SATELLITE OBSERVATIONS OF ClO SATELLITE OBSERVATIONS OF ClO IN THE SOUTHERN HEMISPHERE STRATOSPHERE IN THE SOUTHERN HEMISPHERE STRATOSPHERE

Page 36: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

WHY THE HIGH ClO IN ANTARCTIC VORTEX?WHY THE HIGH ClO IN ANTARCTIC VORTEX?Release of chlorine radicals from reactions of reservoir species in Release of chlorine radicals from reactions of reservoir species in

polar stratospheric clouds (PSCs)polar stratospheric clouds (PSCs)

Page 37: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

PSC FORMATION AT COLD TEMPERATURESPSC FORMATION AT COLD TEMPERATURES

PSC formation

Frost point of water

Page 38: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

HOW DO PSCs START FORMING AT 195K?HOW DO PSCs START FORMING AT 195K?HNOHNO33-H-H22O PHASE DIAGRAMO PHASE DIAGRAM

Antarcticvortexconditions

PSCs are not water but nitric acid trihydrate (NAT) clouds

Page 39: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

DENITRIFICATION IN THE POLAR VORTEX:DENITRIFICATION IN THE POLAR VORTEX:SEDIMENTATION OF PSCsSEDIMENTATION OF PSCs

Page 40: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

CHRONOLOGY OF ANTARCTIC OZONE HOLECHRONOLOGY OF ANTARCTIC OZONE HOLE

Page 41: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

TRENDS IN GLOBAL OZONETRENDS IN GLOBAL OZONE

Mt. Pinatubo

Page 42: Stratospheric Chemistry EPS 133 28 March – 04 April 2011
Page 43: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

LONG-TERM COOLING OF THE STRATOSPHERELONG-TERM COOLING OF THE STRATOSPHERE

Sep 21-30, 25 km, 65-75˚S

Increasing CO2 is expected to cool the stratosphere

Page 44: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

TRENDS IN POLAR OZONETRENDS IN POLAR OZONECould greenhouse-induced cooling of stratosphereCould greenhouse-induced cooling of stratosphereproduce an Arctic ozone hole over the next decade?produce an Arctic ozone hole over the next decade?

Race between chlorine decrease and climate change

Page 45: Stratospheric Chemistry EPS 133 28 March – 04 April 2011

SKIN CANCER SKIN CANCER EPIDEMIOLOGY EPIDEMIOLOGY PREDICTIONSPREDICTIONS