1/26
Looks like no tags are added yet.
Name | Mastery | Learn | Test | Matching | Spaced | Call with Kai |
|---|
No analytics yet
Send a link to your students to track their progress
Main processes that produce O3 (includes loss reactions)
Chapman Mechanism (over-predicts O3)
O 3P (O) and O2 (+ M)
O2 + hv → 2 O
O + O3 → 2 O2
O3 + hv → O + O2
catalytic cycles
X + O3 → XO + O2
XO + O → X + O2
net = O + O3 → 2 O2
X = NO, HO, H, HO2, Cl
Major source of HOx
H2O, CH4
Major source of ClOx
CFCs + hv
Majour source of NOx
N2O + O(1D)
Major sink of ClOx
HCl
Major sink of HOx + NOx
HONO2
Resevoir for ClOx + NOx
ClONO2
Resevoir of HOx
H2O2
Where does HOx dominate with O3 production
lower stratosphere due to most H2O
where does NOx dominate O3 production
middle stratosphere as needs high levels of O(1D) to react with N2O
where does ClOx dominate O3 production
upper stratosphere, high energy photons needed to dissociate CFCs
What is the altitude range for the stratosphere
20-50 km
how is the mixing rate in the stratosphere
slow
[M]z =
[M]0 exp(-z/H)
average Mr of air
28.9 g mol-1
mixing timescale horizontal on Earth
1-2 weeks
mixing timescale vertically on Earth
6 months (from equator)
why is the stratosphere dry
too cold for water, it freezes out
at what altitude does [O3] peak
around 40 km
how do [CH4] and [N2O] change with altitude
generally constant initially then slopes to lower concentration and plateaus
Equation for column of a mixed gas
[X]z H (all in cm)
J(i) =
φ(i,λ) F(λ) σ(i,λ)
F(λ) =
F(TOA) exp(-OD)
Optical depth, OD, =
Σσ(i,λ) x column(i)
what wavelength penetrates to the troposphere
λ>300 nm
Chapman Cycle and its limit
O2 + hv → O + O
O + O2 + M → O3 + M
O3 + hv → O + O2
O + O3 → O2 + O2
it over-predicts the amount of O3
Ox family
O (3P) + O3