chapman mechanism for stratospheric ozone (1930)

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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 O 3 O 2 slow slow fast Odd oxygen family [O x ] = [O 3 ] + [O] R2 R3 R4 R1

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CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930). Odd oxygen family [O x ] = [O 3 ] + [O]. slow. R2. R1. O 2. O O 3. fast. R3. R4. slow. Lifetime of O atoms:. STEADY-STATE ANALYSIS OF CHAPMAN MECHANISM. …is sufficiently short to assume steady state for O:. - PowerPoint PPT Presentation

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Page 1: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

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 2: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

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

Ox

Page 3: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

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

O2+hv O3+hv

Page 4: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

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 5: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

CHAPMAN MECHANISM vs. OBSERVATIONCHAPMAN MECHANISM vs. OBSERVATION

-3

shapedeterminedby k1nO2

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

Page 6: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

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 7: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

WATER VAPOR IN STRATOSPHEREWATER VAPOR IN STRATOSPHERE

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

                             

H2O mixing ratio

Page 8: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

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

radicalsradicals

Page 9: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

NITROUS OXIDE IN THE STRATOSPHERENITROUS OXIDE IN THE STRATOSPHERE

                             

H2O mixing ratio

Page 10: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

• Initiation N2O + O(1D) 2NO• Propagation

NO + O3 NO2 + O2 NO + O3 NO2 + O2

NO2 + h NO + O NO2 + O NO + O2

O + O2 + M O3 + M

Null cycle Net O3 + O 2O2

• Termination RecyclingNO2 + OH + M HNO3 + M HNO3 + h NO2 + OH

NO2 + O3 NO3 + O2 HNO3 + OH NO3 + H2O

NO3 + NO2 + M N2O5 + M NO3 + h NO2 + O

N2O5 + H2O 2HNO3 N2O5 + h NO2 + NO3

O3 loss rate:

32

[O ]2 [NO ][O]

dk

dt

Ozone loss catalyzed by nitrogen oxide (NOOzone loss catalyzed by nitrogen oxide (NOxx ≡ NO + NO ≡ NO + NO22) )

radicalsradicals

Page 11: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

ATMOSPHERIC CYCLING OF NOATMOSPHERIC CYCLING OF NOxx AND NO AND NOyy

Page 12: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

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

Gas-phasechemistryonly

Page 13: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

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

Page 14: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

Ozone loss catalyzed by chlorine (ClOOzone loss catalyzed by chlorine (ClOxx ≡≡ Cl + ClO) radicals Cl + ClO) radicals

• Initiation: Cl radical generation from non-radical precursors (e.g., CFC-12)

CF2Cl2 + h CF2Cl + Cl

• Propagation:

Cl + O3 ClO + O2

ClO + OCl + O2

Net: O3 + O 2O2

• Termination: Recycling:

Cl + CH4 HCl + CH3 HCl + OH Cl + H2O

ClO + NO2 + M ClNO3 + M ClNO3 + hCl + NO3

O3 loss rate: 3[O ]2 [ClO][O]

dk

dt

Page 15: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

ATMOSPHERIC CYCLING OF ClOATMOSPHERIC CYCLING OF ClOxx AND Cl AND Clyy

Page 16: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

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

Page 17: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

CHLORINE PARTITIONING IN STRATOSPHERECHLORINE PARTITIONING IN STRATOSPHERE

Page 18: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

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 19: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

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

Page 20: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

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

Page 21: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

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 22: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

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 23: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

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

Page 24: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

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 25: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

PSC FORMATION AT COLD TEMPERATURESPSC FORMATION AT COLD TEMPERATURES

PSC formation

Frost point of water

Page 26: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

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 27: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

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

Page 28: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

CHRONOLOGY OF ANTARCTIC OZONE HOLECHRONOLOGY OF ANTARCTIC OZONE HOLE

Page 29: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

TRENDS IN GLOBAL OZONETRENDS IN GLOBAL OZONE

Mt. Pinatubo

Page 30: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)
Page 31: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

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 32: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

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 33: CHAPMAN MECHANISM FOR STRATOSPHERIC OZONE (1930)

SKIN CANCER SKIN CANCER EPIDEMIOLOGY EPIDEMIOLOGY PREDICTIONSPREDICTIONS