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Subject: Polar Ozone Hole
Why is the Ozone Hole only over the North and South Poles, and
not distributed evenly over the earth's atmosphere?; Where is the ozone hole
and how fast is it expanding?
A number of processes and effects that occur simultaneously are
believed to be causing seasonal polar ozone depletion known commonly
as the "Ozone Hole". These include:
- the natural chemical reactions responsible for the production and
destruction of ozone in the stratosphere (middle atmosphere)
- the seasonal variations in incident sunlight on the planet
- "special" features of polar weather that isolates this region of the atmosphere from the rest of the planet during part of the year
- the addition to the atmosphere
of ozone depleting chemicals through human activities
- the pressence of "active surfaces" in the polar statosphere upon
which ozone destruction reactions can be enhanced. This includes volcanic aerosols and polar stratospheric clouds.
To understand its distribution in the atmosphere, you must first know what
ozone is and how it is naturally created/destroyed. Ozone is a molecule
composed of 3 atoms of oxygen (O3). The "normal" oxygen we breath
has 2 atoms of oxygen in it (O2).
Ozone is constantly produced and destroyed by chemical reactions in
the upper atmosphere that involve the breaking of O2 into two O atoms
that then react with more O2 to make O3. Oxygen atoms are a type of "free
radical", which is an atom or molecule with a very reactive electron on it.
Light of ultra-violet wavelengths (around 300 nm)
exites O2 and O3 molecules to the proper energy to allow both production
and destruction reactions of O2 and O3 to proceed. These reactions
normally absorb much of the UV radiation the sun directs towards us,
protecting the Earth's surface from its harmful effects. The ozone
reaction is actually more complex then the way I've just described it
for two reasons: 1) it requires mediator molecules that help the
reactions along by transferring some of the energy between the reacting
molecules and 2) other chemical species can get involved, including
other "free radicals" such as Cl and NO.
Ozone can be found in a number of locations in the atmosphere but here I
restrict the discussion to statospheric ozone.
Nature set up a balance for the production and destruction of ozone in
the stratosphere by making available all the materials involved in the
chemical reactions and keeping their concentrations relatively constant
with time. One natural phenomenon that can disrupt this balance is
a volcanic eruption that sends gasses and volcanic ash into the stratosphere.
Not all eruptions do this but particularly violent ones (such as Mt. Pinatubo)
can add particles to the upper atmosphere that will affect the ozone budget
for some period of time.
Why does the amount of ozone vary in the statosphere?
Under normal conditions, the amount of stratospheric ozone depends on the
amount of sunlight reaching a certain geographic area of the atmosphere.
The seasonal variation is low in low lattitudes because sunlight is fairly
constant year-round. In high latitudes, sunlight goes way down in the winter
months. Ozone typically "builds up" to higher values over the poles during
the winter and early spring in each hemisphere. Because this season is
offset by 6 months in the Northern and Southern hemispheres, the effect is
seen at the North and South poles roughly 6 months apart.
How have humans affected the balance of ozone in the stratosphere?
Human use of materials that themselves can destroy ozone or that can be transformed in the atmosphere into ozone depleting chemicals has upset
the natural balance in the stratosphere such that degredation of
ozone is favored relative to production. Sources of halogens (Cl, F, Br)
such as widely used chloroflorocarbons (CFCs) have probably been an important
factor. Freon is one class of CFC that became widely used in
coolant systems soon after it was invented in the 1940s. Another pollutant
we have added to the upper atmosphere that affects ozone are nitrogen oxides
from air plane exhaust.
So, above and beyond, the seasonal variations in ozone that are more
pronounced at the poles, why do the enhanced ozone holes due to human
activities occur over the poles? The air masses above the poles become
isolated from the rest of the atmosphere during their winter and early
spring seasons due to a phenomenon known as the "polar
vortex". In simplest terms, this vortex is a spinning, funnel shaped
region of the atmosphere that forms in late fall and early winter over
a pole, allowing chemical reactions in the enclosed air mass to be enhanced
due to the lack of mixing with other, lower latitude, air masses.
The effect of the pollutants we have added to the atmosphere are thus
enhanced in these isolated regions of the atmosphere. The
Antarctic vortex over the South Pole is more effective at isolating this
region of the atmosphere during the austral winter than is the
corresponding arctic vortex.
A second feature of the polar stratosphere that is unique and probably
aids the polar ozone depletion is polar stratospheric clouds.
These very high altitude clouds are composed of ice crystals, sometimes
greatly enriched in nitrogen oxide specis ("NOx") that can enhance the ozone
degredation reactions discussed above. These ice particles can react with
various forms of Chlorine in the atmosphere and accumulate the molecule
ClONO2, which is a source of ozone depleting Cl radicals.
Once spring time comes, this ClONO2 decomposes and
allows ozone degredation reactions can occur.
Where is the ozone hole and how fast is it expanding?
What scititst usually mean when they speak of the "ozone hole" is an area over
the south pole where lower than normal levels of ozone have been detected. As
discussed above, the amount of ozone in thus layer varies naturally throughout
the year because it is formed and destroyed by chemical reactions that require
light. So the ozone hole is more intense when there is sunlight over the south
pole then where then is darkness (i.e., the austral winter). The size of the
hole also changes (in some years it stretches to lower latitudes as the hole
size increases). Human activities have made the hole much more intense, but as
far as we know there was always a lower amount of ozone over the south pole (and
to a lesser extent over the north pole too) before human activities altered the
composition of the atmosphere. A second, related effect on the ozone layer is
ozone depletion at lower latitudes. This means that the ozone layer has also
thinned in the temperate and tropical zones on Earth.
The images below (courtersy of NASA) provide some additional details about
location and size of the hole.
|| This first image shows an image of the ozone hole using
false colors based on the amount of ozone in the stratosphere as measured by
satellites (a Dobson unit is a measure of the ozone concentration). There are
scale bars on each image. In the first image, deep blue colors signify the
The picture below shows how the hole has changed over time at the
maximum annual hole size (which happens in october). The lowest ozone is
shown with purple colors in this image. The intensity of the holes varies with
time, but overall things looked like they were getting worse over the time
period in this figure. Since that time, the hole has generally gotten less
intense, but it is still easy to detect and ozone depletion well beyond
what we expect naturally.
The signs are good that reduced human use of
some of the worst ozone-depleting halocarbon chemicals are allowing the
hole to slowly repair, but it may take decades (it took a few decades for the
hole to develop after halocarbon refrigreants were introduced during WWII).
Also, there are lots of variables that affect the natural inputs of halocarbons
to the atmosphere as well as volcanic particles, which also affect the ozone
production and destruction reactions in the stratosphere. Plus, other
halocarbons are still widely used today for things like fumigation, fire fighting,
and coolants. So it is not possible to say with certainty that the hole will
continue to decrease, or if we must get used to a somewhat more intense hole
and thinner global ozone layer moving forward from here.
There is still much to be learned about the details of ozone distribution
in the stratosphere. Undoubtedly, much of what we still don't know will
be discovered as additional scientific studies are conducted and the
data is collected and interpreted.
Dr. Ken Rubin, Professor
Department of Geology and Geophysics
University of Hawaii, Honolulu HI 96822
file created, Apr 1997, updated May 2000 and Oct 2008
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