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4. The ozone layer and the ozone hole
Ozone7 is a
compound of three oxygen atoms, O3, rather than the usual oxygen molecule of two atoms, O2.
In high concentrations it is a bluish green gas that is strongly
oxidizing and irritating. It is quite toxic, and while it makes
the air smell fresh after thunderstorms, where it occurs
transiently in small concentrations, it is a common component of
air pollution. Its natural concentration on the Earth’s surface
is only a few parts per million (Ozone Hole).
In 1879 Cornu suggested the sharp drop off in transmission of
light from the Sun below 300 nm wavelengths was due to
atmospheric absorption. In 1880 Hartley postulated the existence
of a layer above the lowest region of the atmosphere in which
ozone absorbed Solar ultraviolet radiation at wavelengths
between 200 and 300 nm. The lowest region of the atmosphere is
now called the troposphere8, and the region postulated by Hartley
is now known as the stratosphere. In 1921 Dobson9 and Linderman
discovered the temperature in the stratosphere increased with
height in contrast to the troposphere where increasing altitude
leads to a decrease in temperature (Austr. Gov, 2006). They
concluded radiative processes dominate in the stratosphere and
the source of energy was from the absorption of Solar
ultraviolet radiation by ozone. Figure 7 shows the relationship
of the troposphere and the stratosphere.

Figure 7. The relationship between the
troposphere, the stratosphere, and the ozone layer. From:
http://amap.no/acia/Files/Ozone-Atmosphere_150.jpg
Ozone is created in the stratosphere by the photo-dissociation
of O2, liberating free oxygen atoms, O, which can
combine with another oxygen molecule to produce ozone, O3. To dissociate an oxygen molecule requires 5.08 eV (Pauling,
1949). This is equivalent to the energy of an ultraviolet photon
with a wavelength of approximately 243 nm. Ultraviolet photons
from the Sun with wavelengths shorter than ~ 240 nm thus are
involved in the dissociation of oxygen molecules in the
stratosphere where effectively all the shortwave length UVR is
absorbed. The free oxygen atoms liberated quickly combine with
oxygen molecules to form ozone.
Ozone itself is dissociated by
light with wavelengths less than 1100 nm into O2 and O, and it
thus absorbs much of the remaining UVR not involved in the
dissociation of oxygen molecules themselves. The oxygen atom
freed up by the dissociation of ozone quickly finds another O2
molecule to pair up forming an ozone molecule anew. The final
result is absorption of most of the Sun’s UVR with its energy
being transformed into thermal energy in stratosphere. This
mechanism thereby protects the plants and animals on the Earth’s
surface from dangerous or lethal levels of ultraviolet
radiation.
Dobson designed and built a number of precise ultraviolet
spectrographs to study the stratospheric ozone. His measurements
of ozone’s seasonal and latitude variations beginning in the
1920’s helped established the basic patterns of stratospheric
ozone recognized today. Also, he quantified the vertical column
density of ozone in the atmosphere. Today, the thickness of the
atmospheric ozone layer is measured in Dobson units (DU), one
unit of which is defined to be 0.01 mm thickness of ozone at
standard temperature and pressure (STP: 00 Celsius;
one atmosphere or 1013.25 milibars). It is the thickness of the
ozone layer if it were fully compressed in the Earth’s
atmosphere. A normal range is 300-500 DU, which translates to a
compressed thickness of 3 to 5 mm (Ozone Hole).
Atmospheric ozone is spread from an altitude of 10-12 km to 40
km with the maximum at 17-25 km. This region is known as the
ozone layer which is now monitored extensively from the ground
and from space. Even in the ozone layer, ozone is not very
common existing as only one part in 100,000. A global network of
Dobson spectrophotometers was established during the
International Geophysical Year in 1956-1957. Today, at least 150
Dobson Spectrophotometers are in use worldwide making daily
observations. These measure the intensity of the Solar UV
radiation at two different wavelengths, one of which is absorbed
by the ozone layer and one of which is not.
The ozone in the ozone layer is known as “good ozone” while
ozone created near the ground is sometimes called “bad ozone.”
The latter is formed when various compounds, particularly
nitrogen oxides, emitted by cars, power plants, industrial
plants, refineries, chemical plants, and many other sources
react in the atmosphere in the presence of sunlight to produce
ozone. Bad ozone is particularly a concern in summer when high
temperatures and much sunlight provide the ideal conditions for
its formation. Ozone in more than minimal amounts is damaging to
the lungs (Ozone Hole).
Chlorofluorocarbons (CFCs) are a large family of compounds
containing hydrogen, carbon, chlorine, and fluorine (figure 8).
They were first introduced in the 1930’s as safe non-flammable
and non-toxic refrigerants and spray can propellants. CFCs are
very stable in ordinary circumstances and have been extensively
used as aerosol propellants, refrigerants, solvents, foam
blowing agents, and the like. They can be readily converted from
the liquid to a gaseous form. One common CFC is Freon.

Figure 8. Typical chlorofluorocarbons. From: http://www.ucar.edu/learn/images/cfcmole.gif
Unfortunately, despite their safety record on the ground, CFCs
are extreme environmental hazards, because CFCs released into
the atmosphere make their way to the stratosphere where the
ultraviolet radiation can decompose them into their base
elements. The chlorine reacts with ozone to form O2 and ClO, the
latter of which can react with free oxygen atoms to form more
chlorine:
CFCl3 + UVR -> CFCl2 + Cl
Cl + O3 -> O2 + ClO
ClO + O -> Cl + O2
These reactions not only destroy ozone, but they compete with
the formation of ozone itself. Chlorine stays in the atmosphere
for many years, and one atom of chlorine can destroy thousands
of atoms of ozone (NOAA, 1998). Bromine containing chemicals act
in a similar fashion (Ozone Hole).
In 1995, the Nobel Prize for chemistry was awarded to F.
Sherwood Rowland, Mario Molina, and Paul Crutzen for their 20
plus years of studying the ozone layer. The ozone layer is
critical to life because it absorbs the majority of the Sun’s
UVR. In 1970 Crutzen showed nitrogen oxides NO and NO2 react with stratospheric ozone to hasten its destruction.
These oxides are common air pollutants and occur naturally as
soil microorganisms produce NO2 as part of their
natural metabolic processes. In 1974 Molina and Rowland proposed
that CFCs could be gradually transported through normal air
circulation to the stratosphere where their breakdown would
catalyze ozone destruction (Molina, 1974). This produced an
intense reaction from users and producers of CFCs, but in 1985 a
drastic seasonal depletion of stratospheric ozone over
Antarctica was discovered, the so-called ozone hole (figure 9)
(Science Updates; Ozone Hole).
The ozone hole forms seasonally over Antarctica, because in the
Antarctic spring stratospheric clouds form in exceptionally cold
temperatures. These clouds allow chemical reactions that
transform various chlorine species into forms that are
particularly destructive of ozone. The rare stratospheric clouds
are formed by water and nitric acid at extremely low
temperatures, mainly over Antarctica. The amount of harmful
reactive chlorine over the Antarctica becomes much higher than
at middle latitudes leading to a faster destruction of ozone and
the formation of an ozone hole (NOAA FAQ).
Figure 9. The ozone hole over
Antarctica October 5, 1987. From Science Updates and NASA.
Is the ozone hole a real effect, and is ozone depletion a
concern that should be addressed? Yes. If atmospheric ozone were
to be depleted, high levels of UVR would reach the ground. For
example, McKenzie and colleagues (1999) found that long term
decreases in summertime ozone over Lauder, New Zealand, at 450 south latitude led to substantial increases in peak ultraviolet
radiation. In the summer of 1998-1999, the peak sun burning ultraviolet radiation was 12% more than a decade earlier, whereas UVA radiation which
is not absorbed by the ozone layer, showed no increase. It is
estimated a 1% decrease in ozone leads to up to a 3% increase in
non-melanoma skin cancers (McKenzie, 1999).
The possibility supersonic aircraft and supersonic travel (SST)
might be a threat to the ozone layer was noted by the American
researcher Harold Johnson in 1971. These aircraft would be
capable of releasing nitrogen oxides directly into the ozone
layer at altitudes of 20 km (Science Updates). The United
Nations became involved in the threat to the ozone layer and the
Montreal Protocol10 was signed in 1987. This called for the
complete elimination of CFCs, halons, carbon tetrachloride, and
methyl chloroform by 2000 (2005 for methyl chloroform)11 (EPA).
The first comprehensive satellite monitoring of the ozone layer
was started in 1978 with the Nimbus-7 satellite which carried a
Total Ozone Mapping Spectrometer (TOMS) (figure 9). Today,
stratospheric ozone is monitored by Dobson spectrophotometers
throughout the world, by ozone sondes, balloon borne instruments
that continuously measure ozone concentrations as they ascend
through the atmosphere as high as 30 km, and by satellite
observations. Satellites have provided a nearly continuous
record of ozone observations since October 1978. For example,
the Australian Government Bureau of Meteorology Atmosphere Watch
Section routinely monitors total ozone data from the Tiros
Operational Vertical Scanner (TOVS) and other information from
the U.S. National Oceanic and Atmospheric Administration (NOAA)
polar orbiting satellites as well as from China’s FY-1D
satellite (Austr. Gov, 2006). The currently active NOAA polar
orbiting satellites are NOAA 12, 15, 16, and 17.
There is a confusing array of satellites launched by the United
States, the European Space Agency (ESA), Russia, Japan, China,
and India which monitor the Earth’s weather. One of the most
advanced satellites is the Aura mission which was launched on
July 15, 2004 as part of NASA’s Earth Observing System (EOS). A
prime instrument of Aura is the Ozone Monitoring Instrument
(OMI) contributed by the Netherlands’s Agency for Aerospace
Programs (NVR) in collaboration with the Finnish Meteorological
Institute (FMI). OMI observes Solar backscatter radiation in the
visible and ultraviolet. Aura provides daily global coverage of
the Earth with its 14 orbits a day. OMI is the latest
contributor to the several decades old nearly continuous
satellite ozone monitoring that began with the Nimbus-4 in 1970
and the Nimbus-7 TOMS instrument in 1978 (Aura). A daily ozone
hole watch is available from NASA's Ozone Hole Watch.
Figure 10 shows in graphical form the severity of the ozone hole
since 1979.

Figure 10. Comparative values for the ozone
concentration and the ozone hole size from 1979 to 2013. From Ozone Hole Watch .
There is now speculation that the stratospheric ozone layer will
recover by 2050 to 2070 (Ozone Hole). However, the effect of
ozone on the weather and the effect of ozone on global warming
are unpredictable. Ozone generates heat in the stratosphere by
absorbing the Sun’s ultraviolet radiation and by absorbing
infrared radiation from the troposphere. Falling ozone levels
may somewhat mitigate the effects of global warming, or they may
start a vicious cycle as falling ozone levels decrease
stratospheric temperatures producing conditions that favor even
more ozone depletion (Ozone Hole)
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