Title: What is Actually Important in Atmospheric Chemistry
1What is Actually Important in Atmospheric
Chemistry?
- Ozone - The 'Ozone Problems'
- Oxidation Capacity - Removal of 'Pollutants'
- Free Radicals - The 'Driving Force'
- Greenhouse Gases - Chemistry Radiation Link
- Aerosol - 'Liquid - Solid'
2Stratospheric ozone chemistry
Overview
- Stratospheric O3 Why do we care?
- Short historic overview
- Typical ozone profile
- The Chapman cycle
- Odd oxygen family
- Steady state solutions
- Global ozone distributions and implications for
circulation - Beyond Chapman Catalytic destruction cycles
- The polar ozone hole
- Ozone hole chemistry
3Ozone in the Atmosphere
4The solar spectrum
5Stratospheric ozone Why do we care?
6Penetration of short-wave UV radiation
7Solar radiation flux, absorption spectra of O2
and O3 and absorption in the atmosphere
8UV Penetration depth
350-315 nm
315-285 nm
lt285 nm
9The Dobson unit (DU)
- Bring all the ozone in the atmospheric column to
the surface and measure the height of the layer
at 1 atm and 273K - 1DU equals 10-5 m of ozone
- Thus 100 DU amounts to 1 mm of O3
- Typical atmospheric values 250 400 DU
10Short historic review Discovery of O3
1840 Officially named as a chemical in 1840 by
Christian Schönbein, after he noted that it had a
smell that was similar to that of phosphorus when
exposed to air 1882 Chappuis discovers O3
absorption in the visible spectral range (ozone
liquifaction). Blue colour of the sky?? 1890 Sir
William Huggins discovers a new line group in the
spectrum of Sirius (long-wave UV absorption of
O3)
Absorption cross section of O3 Different parts of
the spectrum are named after the discoverers
Hartley-, Huggins- und Chappuis Bands.
11Short historic review Measurement of O3
1925 Gordon Dobson develops the
Dobson-Spectrophotometer to measure thickness of
ozone layer
Intensity measurement with a Dobson-spectrograph U
se several wavelength pairs
Absorption cross section (cm2)
wavelength (nm)
12Dobson-Animation
13Balloon flights by E. Regener, Stuttgart, 1934
First direct measurement of the ozone layer
14Ozone profiles
3,000 ppb
lt100 ppb
tropopause
15The ozone layer in different units
altitude (km)
concentration (molec/cm3)
16The Origin of Stratospheric Ozone
The Chapman Cycle, introduced in the 1920s by S.
Chapman, to explain the ozone layer. O2 h?
? O(3P) O(3P) Rate 1 JO2O2 O(3P) O2
M ? O3 M Rate 1 k2OO2M O3
h? ? O(3P) O2 (3?) Rate 3 JO3O3
? O(1D) O2 (1?) ..........O(1D) M ?
O(3P) M (quenching) O(3P) O3 ? O2
O2 Rate 4 k4OO2 O(3P) O(3P) M ?
O2 M Rate 5 k5OOM
llt242nm
llt1130nm
llt320nm
JO2 see figure k2 6 ? 10-34 ? (300/T)2.3 ?
M k4 8 ? 10-12 exp(-2060/T) cm3molec-1s-1 JO3
? 5 ? 10-4 s-1 (see figure, only slight
dependency on altitude) T absolute temperature
(K)
17SPECTRUM OF SOLAR RADIATION vs. ALTITUDE
O3 hn
O2 hn
18The O2- und O3- Photolysis frequencies (Jc2,
Jc3), s-1
19O3 formation figure
20Slow and fast reactions
The Chapman Cycle, introduced in the 1920s by S.
Chapman, to explain the ozone layer. O2 h?
? O O Rate 1 JO2O2 O O2 M ? O3
M Rate 2 k2OO2M O3 h? ? O O2
Rate 3 JO3O3 O O3 ? O2
O2 Rate 4 k4OO2
llt242nm
slow
fast
llt320nm
fast
slow
21The Chapman differential equations
1. Rate of change of O (short for
O(3P)) d/dtO 2?jO2?O2 jO3?O3
k2?O?O2?M k4?O?O3 2. Rate of change
of O3 d/dtO3 k2?O?O2?M JO3?O3
k4?O?O3 3. Rate of change of OX d/dtOX
2?jO2?O2 2?k4?O?O3
22Chemical steady state
Chemical steady-state assumed for species if
production and loss rate constant over
lifetime Lifetime of shortest-lived species ?O
O / k2OO2M 1 / k2O2M ? secs ?s.s.
for O between JO3 and R2 ( neglecting slow R1
and R4)
23Steady state for O, only fast reactions
d/dtO jO3?O k2?O?O2?M 0
O/O3 JO3/ k2MO2
O3
O/O3 ltlt1
Observations agree closely with Chapman
O
Ox O O3 ? O3
24Ox steady state
Effective O3 lifetime ? ?Ox ?Ox
Ox/2k4OO3 ? 1/ 2k4O
?Ox lt 1 day in the upper stratosphere ? steady
state assumption OK ?Ox years in lower
stratosphere
Steady state for Ox 2JO2 O2
2k4OO3 ?O3 (JO2k2/JO3k4)1/2 ?O2na3/2
?Ox
25Families in the Atmosphere
The "Odd Oxygen" Family Oodd OX O
O3 Formation of OX O2 h? ? O(3P) O(3P)
(Jc2) Destruction of OX O(3P) O3 ? O2
O2 (Rc3) O(3P) O(3P) M ?O2
M (Rc1)
26Steady-State solutions for Chapman ozone
27Analytical solution not trivial
O3 (JO2k2/JO3k4)1/2 ? O2na3/2
- JO2(z) and JO3(z) are photolysis rate constants
(not reaction rate constants) - J ?? qX(?)?X (?)I?d ?
- I? I?,? e-?/cos?
- ?? ?(?O2 O2 ?O3 O3)dz
Actinic flux depends on O2 O3 above
Solar zenith angle
Optical depth
28Energy distribution in the stratosphere(Chapman
function)
29Chapman and measurements
Good qualitative agreement
Upper stratosphere flaw in theory
Maximum vertical dependence of Ox production
2JO2O2 O2 decreases with z JO2 increases
with z
Lower stratosphere s.s. not expected because of
long ?Ox ALSO DYNAMICS
What is missing? Source or sink?
30Ozone production rate and distribution
Production rate in molec cm-3 s-1, calculated
based on O2 photolysis rate
N-S asymmetry
Distribution in 1012 molec cm-3
31Distribution and annual cycle of O3 column
density (in DU)
32Brewer-Dobson circulation
- Observation
- O3 columns are smallest in tropics despite this
being the main stratospheric O3 production region
- Explanation
- Rising tropospheric air with low ozone
- B-D circulation transports O3 from tropics to
mid-high latitudes
- Other comments
- O3 maxima occur toward high latitudes in late
winter/early spring - the result of the
descending branch of the B-D circulation - Virtually no seasonal change in the tropics
- More accurate data has led to improvements in our
understanding of this simple circulation pattern.
33Atmospheric motion and mean CH4 mixing ratio
34Age of air in the stratosphere
35Turbulent diffusion constant KM, cm2s-1
36Age of air in the stratosphere
Waugh and Hall 2002
37Stratosphere-troposphere exchange
38Energy balance
Radiative heating and cooling in the stratosphere
39Catalytic O3 destruction cycles
Good qualitative agreement between Chapman theory
and measurements, but factor of 2 difference
40Radical reactions in the atmosphere
Does that also happen in the atmosphere?
41CATALYTIC CYCLES FOR OZONE LOSS
Chapman got it almost right
General Idea
O3 X ? XO O2 O XO ? X O2 Net O3
O ? 2 O2 X is a catalyst
The catalyst is neither created nor destroyedbut
the rate for the catalytic cycle odd-o removal
in this case depends on catalyst concentrations
42Hydrogen oxide (HOx) radicals (HOx OH HO2)
( H??)
Source from troposphere
- Initiation H2O O(1D) ? 2OH
- Propagation through cycling of HOx radical family
(example) - OH O3 ? HO2 O2
- HO2 O3 ? OH 2O2
Net 2O3 ? 3O2 - Termination (example)
- OH HO2 ? H2O O2
HOx is a catalyst for O3 loss but not the only
one
43Nitrogen oxide (NOx)radicals (NOx NO NO2)
- 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 Recycling
- NO2 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
44ATMOSPHERIC CYCLING OF NOx AND NOy
45DESTRUCTION OF O3 BY NOX
- Production Natural NOx by
- N2O O(1D) - well understood source
- Loss Dominant sink is deposition to troposphere.
Residence time for air is 1-2 years. Loss rate
well constrained - Cycling O3 loss related to NOy/NOx ratio. Under
most conditions s.s. between NOy is a good
approximation
NOx catalytic cycle reconciled Chapman theory
with observations1995 Nobel Prize (Paul Crutzen)
46STRATOSPHERIC DISTRIBUTION OF CFC-12
47NOMENCLATURE OF CFCs
- CFC-01234a where 0 number of double bonds (
omitted if zero ) - 1 Carbon atoms - 1 ( omitted
if 0 ) - 2 Hydrogen atoms 1
- 3 Fluorine atoms
- 4 Chlorine atoms replaced by
Bromine ("B" prefix added ) - a letter added to identify
isomers, the "normal" isomer - in any number has the
smallest mass difference on each - carbon, and a, b, or c are
added as the masses diverge - from normal.
- CFC-11 CCl3F trichlorofluoromethane
- CFC-12 CCl2F2 dichlorodifluoromethane
- CFC-113 CCl2F-CClF2 1,1,2-trichlorotrifluoro
ethane - HCFC-22 CHClF2 chlorodifluoromethane
- HCFC-123 CHCl2-CF3 2,2-dichloro-1,1,1-trifl
uoroethane - HCFC-123a CHClF-CClF2 1,2-dichloro-1,1,2-trifl
uoroethane - HFC-23 CHF3 trifluoromethane
- R-20 CHCl3 chloroform
- R-22B1 CHBrF2 bromodifluoromethane
- R-1120 CHClCCl2 trichloroethylene
48CATALYTIC CYCLES FOR OZONE LOSSChlorine (ClOx
Cl ClO) radicals
- Initiation
- CF2Cl2 hn g CF2Cl Cl
- Propagation
- Cl O3 g ClO O2
- ClO O g Cl O2
- Net O3 O g 2O2
-
- Termination Recycling
- Cl CH4 g HCl CH3 HCl OH g Cl H2O
- ClO NO2 M g ClNO3 M ClNO3 hn g ClO NO2
O3 loss rate
Discovery of the halogen catalytic cycles 1995
Nobel Prize (Mario Molina and Sherwood Rowland)
49ATMOSPHERIC CYCLING OF ClOx AND Cly
50STRATOSPHERIC OZONE BUDGET FOR MIDLATITUDES
BASED ON 1980s SPACE SHUTTLE OBSERVATIONS
Gas-phase chemistry only
What is the effect of increasing stratospheric
NOx on the rate of ClOx-catalyzed ozone loss?
51ATMOSPHERIC TREND OF CFC-11
CFC production Is banned
Montreal protocol
52OZONE COLUMN TREND, 60oS-60oN WMO, 1998
Stabilization of chlorine?
Chlorine Or dynamics?
Pinatubo
53RECENT RISE IN HFCs (CFC REPLACEMENT PRODUCTS)
54OZONE TREND AT HALLEY BAY, ANTARCTICA
55THE ANTARCTIC OZONE HOLE
Southern hemisphere ozone column seen from TOMS,
October
DU
1 Dobson Unit (DU) 0.01 mm O3 STP 2.69x1016
molecules cm-2
56OZONE HOLE IS A SPRING PHENOMENON
57Vertical structure of the Ozone hole
Ozone profiles in August (Antarctic winter) of
1996 and October (Antarctic spring) of 1997,
Nardi et al. 1999
58What is missing in O3 chemistry?
- Problem at the low zenith angles in polar spring
there is not enough O2 photolysis to produce
sufficient O atoms - But O atoms needed for most catalytic cycles
Solution ClO dimer cycle ClO ClO M g
ClOOCl M ClOOCl h?? g ClOO Cl ClOO
?? g Cl OO M Cl O3 g ClO O2 (2?)
Net 2O3 g 3O2
No O atoms needed!!! ClOOCl breaks at Cl-O
bond 70 of total O3 loss in O3 hole!
59O3 and ClO
60SEASONAL TREND OF ClO IN THE POLAR VORTEX
61Additional O3 destruction cycle
- Cl O3 g? ClO O2
- Br O3 g? BrO O2
- ClO BrO g? Cl Br O2
- Net 2O3 g 3O2
30 of O3 destruction in O3 hole conditions
62Why is there so much ClO over Antarctica?
???
ClNO3 HCl g Cl2 HNO3 Cl2 h? g?2 Cl
63PSC BILD2
64PSCs OVER KIRUNA, SWEDEN (SOLVE MISSION)
65PSC FORMATION vs. TEMPERATURE
66ACTIVATION OF CHLORINE IN THE ANTARCTIC VORTEX
67HNO3-H2O PHASE DIAGRAM SHOWING STABLE CONDENSED
PHASES AT EQUILIBRUM WITH VAPOR
Antarctic vortex conditions
68DENITRIFICATION IN THE POLAR VORTEX
69CHRONOLOGY OF ANTARCTIC OZONE HOLE
70Ozone at mid latitudes
71The Gradual Decrease of Global Stratospheric O3
(W. Attmannspacher in Graedel and Crutzen, 1994)