Meteo 465 – The Middle
Atmosphere
Mid-term Open-book Exam
Assigned:
10:00 AM, 07 March 2003
Due:
10:00 AM, 24 March 2003
You should be able to answer all the questions using
the material in the chapter “Stratospheric Chemistry - Perspectives in Environmental Chemistry”, your notes, and a
reference text for things like atomic masses, air densities, etc.. You may consult texts, websites, or other
documents. However, please do not
consult each other.
1.
(15 points) I posed the following
question in class; now I will pose it again on this exam. We know that heterogeneous chemistry at low
temperatures causes rapid ozone loss at wintertime high latitudes, yet air gets
as cold in the stratosphere just above the tropical tropopause as it does in
the wintertime polar lower stratosphere.
In a few hundred words, or less, present your case for why you do or
don’t think that ozone loss in the tropical lower stratosphere is important.
The tropical tropopause does
get as cold as 190 K, especially over Micronesia in January. In addition, there is evidence that very
tenuous Tropical Stratospheric Clouds do form.
However, several factors work against massive stratospheric ozone loss
in this region.
2.
(20 points) It is now clear
from the figure on atmospheric heating vs. altitude that ozone absorption is
mainly responsible for the solar heating near 50 km, much to even my surprise
in class.
a. Using the equation on solar heating by ozone and molecular oxygen
in the web-based notes on Stratospheric Heating and Cooling, demonstrate that
this heating is indeed due to ozone and that it makes sense that that its
maximum heating occurs near 50 km.
b. Show that O3 is more important at 50 km than O2
by estimating the relative heating rates of O3 and O2.
To demonstrate the ozone
heating, we must put numbers in the equation:
dT/dt = (r cp)-1 òl I {sO2(l) [O2] + sO3(l) [O3] }dl
Both the absorption cross
sections and I have wavelength dependences.
In addition, I, [O3], [O2], and r have altitude dependences. We can use Figure 1.8 from the Chemistry
chapter to get I at different wavelengths and altitudes, and use JPL to get the
cross sections for O3 and O2. We must estimate some values, but these estimates turn out to be
unimportant. Thus, the integral becomes
sums over wavelengths, where I used 20 nm bins:
dT/dt = (r(z) cp)-1 S[ I(z,l) {sO2(l) [O2](z) + sO3(l) [O3](z) }]Dl
This crude model worked
amazingly well. Ozone is clearly
responsible for the heating at 50 km, while O2 plays a rather minor
role there.
3.
(25 points) The fast
photochemistry of OH and HO2.
Equations & figures are in Stratospheric Chemistry – Perspectives in
Environmental Chemistry.
(a.)
Write down the rate equations for OH and HO2 using equations
1-22, 1-26 through 1-31, 1-34 (and assuming that the production of HOx
(OH+HO2) is due to: O3 + hn ® O(1D) + O2,
followed by O(1D) + H2O ® 2OH. Ignore reactions 1-23 and 1-25. Assume that HOCl rapidly photolyzes. Remember that reaction 1-31 is much faster
than the others.
(b.)
Assume that HOx production equals HOx loss by
reaction 1-34. Show that the reactions
that exchange HOx between OH and HO2 are fast compared to
HOx production and loss using Figure 11.
(c.)
Derive the steady-state expression, equation 1-32.
(d.)
Simplify the expression to contain only the dominant terms at 45 km and
at 15 km.
(e.)
There are three ozone-destroying catalytic cycles involving HOx
that are given on pages 23 and 24.
Write down the ozone loss rate expression (d[O3]/dt = ….) for
these HOx catalytic cycles.
(a.)
(b.) Since HOx
production and loss are equal, we can use the OH+NO2 curve in Figure
11 to evaluate the rates of these processes.
We see that they vary from ~2x103 cm-3 s-1
at 15 km to ~104 cm-3 s-1 at 30 km to less
than 103 cm-3 s-1 at 45 km. With the exception of HO2+O below
25 km, all the other reactions are at least ~5 times greater that OH+NO2
for the entire altitude range. We can
therefore safely ignore primary production and loss in examining the balance
between OH and HO2.
(c.) We assume that the
OH+CO is not important except at very low and very high altitudes. To derive the steady-state expression 1-32,
assume that d[HO2]/dt = 0. We could to the same thing for OH. By simple algebra,
(d.) 45 km: From Figure 11, HO2+O3,
HO2+NO. and HO2+ClO << HO2+O. Thus,
15 km: From Figure 11, HO2+O, and HO2+ClO
<< HO2+O3 ~ HO2+NO. Also, OH+O must be much less than OH+O3. Thus,
(e.) Recall that HO2+NO®NO2 + OH actually ends up creating
O3 because NO2 photolyzes to make O, which makes O3. Thus, some of the OH reactions balance this
reaction in the cycle, which is a null cycle for O3 loss. So, we must consider only the HO2
reactions that cause O3 loss, realizing that some of the OH
reactions balance this:
We have assumed that HO2+ClO
is slower than HOCl+hn.
4.
(20 points) Ozone loss in the
polar stratosphere.
(a.)
On page 27, it states “In the lower stratosphere, where [M] = 2x1018
cm-3, cClO = 1 ppbv, cBrO = 7 pptv, the loss rate of
ozone can approach 1 to 3 percent per day in the sunlit parts of the
vortex”. Verify this statement with
calculations.
(b.)
As ClO gets tied up in ClONO2 (due to photolysis of HNO3,
followed by ClO+NO2+M®ClONO2+M), the
ozone destruction by ClO+BrO becomes more important. Assuming the cBrO = 7 pptv and that f
(photolysis) = 0.8, at what value of cClO are the two ozone destruction
terms in equation 1-62 equal?
(c.)
Polar ozone loss requires sunlight to break apart Cl2O2
and species containing bromine. At the
same time, if any HNO3 remains in the gas-phase, it too is
photolyzed, although at a much lower
rate than Cl2O2.
Explain why the photolysis of HNO3 is still effective at
slowing polar ozone loss, even though the photolysis frequency is so small
compared to the photolysis of Cl2O2. Use numbers to support your thoughts.
(d.)
Why is Figure 21 not sufficient to prove that the Antarctic Ozone Hole
is caused by chlorine? Think about what
constitutes proof that a process is occurring?
(a.) The ozone loss is given by the expression:
where fphotlysis
is the fraction of ClOOCl that photolyzes and does not thermally decompose,
while fBrO is the fraction of the reaction that does not form OClO,
which photolyzes to give O back.
Assume T = 200 K. Thus, for [M]=2x1018 cm3
molecule-1 s-1, kClO+ClO = 1.3x10-13
cm3 molecule-1 s-1, and kClO+BrO = 2.9x10-12exp(220/200) + 5.8x10-13exp(170/200)
= 1.0x10-11 cm3 molecule-1 s-1. We find the concentrations by multiplying
the mixing ratios by [M].
so,
where we assume 12 hours of
sunlight so that ClOOCl can be photolyzed.
At these altitudes, O3
is a few ppm (See Figure 21 in the chapter).
Thus, we see that ozone is lost at a few percent per day.
(b.) To find out, set the
two terms equal to each other:
(c.) The photolysis of
ClOOCl is quite fast, about 10-3 s-1, as I said in my
e-mail. In Figure 12, we see that the
photolysis of HNO3 is 3x103/1010 = 3x10-7
s-1. (We divide the rate by the concentration of HNO3 to
get the photolysis frequency.) This
number is 3300 time bigger. However,
the amount of HNO3 is usually as much as 10 times more than that of
ClO. Every molecule of HNO3
results in the formation of NO2, which immediately reacts with ClO
to form ClONO2. Thus for
each ClO molecule, it goes through its ozone-destroying cycle 330 times before
being tied up with NO2 to form ClONO2. Thus, a few times 103 ClO
molecules are tied up into ClONO2 each second, or about 108
cm3 (0.05 ppbv) per day. In
~20 days, all the ClO will be effectively tied up.
(d.) Figure 21 provides a
snap-shot of the ozone and ClO inside and outside the polar vortex, but some
other phenomenon could have been responsible for elevating ClO and depressing O3. By taking several snap-shots over the ozone
hole’s evolution, we can calculate the observed O3 loss rate and
compare it with the calculated O3 loss rate. They agree to about a factor of two, which
gives us confidence that we understand the major loss processes that are
responsible for the Antarctic Ozone Hole.
5. (20 points) The End-of-Mission statement
from the 1994 Airborne Southern Hemisphere Ozone Experiment / Measurements for
Assessing the Stratospheric Effects of Aircraft (ASHOE/MAESA) campaign using the NASA ER-2 high altitude aircraft
contains the following statement:
“Polar air
nearly devoid of ozone was sampled in-situ for the first time inside the vortex
near the 400 K potential temperature surface (about 16 km altitude) on 10 and
13 October. Mid-October is late in the
period of severe ozone depletion over Antarctica. This air contained little O3 (<0.4 ppmv), little or
no ClO (<100 pptv), high NO (1 ppbv), low NOy (2 ppbv), and HCl
equivalent to estimates of total inorganic chlorine (not in the form of CFCs or
CH3Cl) (2.6 ppbv).”
Given that O3 is low, show with words and chemical equations
why each other chemical species are observed to have the values that they
do.
Recall
that most inorganic chlorine is in the forms of Cl, ClO, and ClOOCl as ozone is
being destroyed. What is the time
constant for Cl, ClO, and ClOOCl to be converted into HCl when O3
drops to 0.4 ppmv? (hint: Write down the formation rate for HCl and assume that
all inorganic chlorine is initially in the forms of Cl and ClO and that Cl and
ClO are in steady-state.)
When
most of the O3 is destroyed, there is a shift in which reactions are
most important. First, NO increases relative
to NO2 because the reaction NO+O3®NO2+O2
slows down while the reaction NO2+hn®NO+O remains about the same. Because ClO+NO®Cl+NO2 is now faster, ClO preferentially
reacts with NO and not ClO. Because
ClO+NO®Cl+NO2 is now faster and Cl+O3®ClO+O2
is now slower, the balance of reactive chlorine shifts toward Cl. Hence, the rate of HCl formation by the
reaction Cl+ CH4®HCl+CH3 increases, and reactive chlorine
is rapidly shifted into HCl. This
increased formation of HCl thus rapidly decreases the amount of reactive
chlorine and thus the chlorine ozone-destroying catalytic cycles. It also explains the observations.
The
reaction that determined that lifetime of reactive chlorine in this situation
is:
Cl + CH4 ® HCl + CH3.
Thus,
Cl first-order loss rate is (kCl+CH4[CH4]). From Figure 6.04b in the NASA GSFC
Electronic Textbook, we see that CH4 is about 1 ppm in March at
Northern high latitudes.
This
is equivalent to about 2x1012 molecules cm-3. From JPL, at lets say 220 K, the reaction rate
coefficient for Cl+CH4 is kCl+CH4 = 1.1x10-11exp(-1400/220)
= 2x10-14 cm3 molecule s-1.
We
are not interested in the Cl lifetime alone, but rather, the ClOx
lifetime. We can find this by
considering the relationship between Cl and ClOx. Consider the reactions that are dominant in
this environment:
ClO
+ NO®
Cl+NO2
Cl+
O3 ® ClO+O2
Cl
+ CH4 ® HCl + CH3
In
steady-state,
We
see that the lifetime of ClOx is quite short once ozone has been
lost. Only heterogeneous reactions on
PSCs can reactivate the chlorine, and that is even limited by the lack of ClONO2. Thus, the system simple stops.