Some experts predicted that the depletion
of ozone in the stratosphere due to the exhausts from the SST would produce about 10,000 additional cases of skin cancer in the world.
It is therefore very important to consider the effect of solar proton events on the temporal and spatial distribution
of ozone in the stratosphere.
The meeting was the first large - scale attempt to bridge the gap between scientists and policymakers on a wide range of atmospheric problems, including not just the greenhouse effect but also acid rain and the depletion of the protective layer
of ozone in the stratosphere.
OMPS is a three - part instrument: a nadir mapper that maps ozone, SO2 and aerosols; a nadir profiler that measures the vertical distribution
of ozone in the stratosphere; and a limb profiler that measures aerosols in the upper troposphere, stratosphere and mesosphere with high vertical resolution.
At precisely these altitudes, the amount
of ozone in the stratosphere declined between three and six months after the eruption.
Dr. Okano is the first to observe height profiles
of ozone in the stratosphere from the ground with laser heterodyne spectroscopy.
And, «fluctuation
of ozone in the stratosphere is likely a natural phenomenon because solar radiation is a fluctuating event.»
52 • Immune system suppression Natural Capital Degradation Effects of Ozone Depletion Human Health • Worse sunburn • More eye cataracts • More skin cancers • Immune system suppression Food and Forests • Reduced yields for some crops • Reduced seafood supplies from reduced phytoplankton • Decreased forest productivity for UV - sensitive tree species Wildlife • Increased eye cataracts in some species • Decreased population of aquatic species sensitive to UV radiation • Reduced population of surface phytoplankton • Disrupted aquatic food webs from reduced phytoplankton Figure 20.21 Natural capital degradation: expected effects of decreased levels
of ozone in the stratosphere.
Destruction
of ozone in the stratosphere takes place as quickly as formation of ozone, because the chemical is so reactive.
The presence of a layer
of ozone in the stratosphere is the cause of the temperature inversion that forms at the tropopause.
As an example, variations in the flow of both UV radiation and atomic particles that accompany changes in overall solar activity alter the amount
of ozone in the stratosphere.
60 • Immune system suppression Natural Capital Degradation Effects of Ozone Depletion Human Health • Worse sunburn • More eye cataracts • More skin cancers • Immune system suppression Food and Forests • Reduced yields for some crops • Reduced seafood supplies from reduced phytoplankton • Decreased forest productivity for UV - sensitive tree species Wildlife • Increased eye cataracts in some species • Decreased population of aquatic species sensitive to UV radiation • Reduced population of surface phytoplankton Figure 20.21 Natural capital degradation: expected effects of decreased levels
of ozone in the stratosphere.
Not exact matches
This «would create a persistent layer
of black carbon particles
in the northern
stratosphere that could cause potentially significant changes
in the global atmospheric circulation and distributions
of ozone and temperature,» they concluded.
It would provide important insight into how much SRM would reduce radiative heating, the concentration
of water vapor
in the
stratosphere, and the processes that determine water vapor transport — which affects the concentration
of ozone.
Recently, additional
ozone production mechanisms have been proposed to resolve the
ozone deficit problem, which arises from greater
ozone destruction than production
in several photochemical models
of the upper
stratosphere and lower mesosphere.
At present, naturally - emitted VSLS account for around 90 %
of the total
ozone loss caused by VSLS
in the lower
stratosphere.
Such sulfuric acid aerosols are already responsible for the bulk
of nacreous clouds that form
in the polar
stratosphere; added particles would just amp up the natural process (although it might also amp up damage the
ozone layer).
This is what's known about the dynamics
of the
stratosphere: Increasing clouds
of low - lying
ozone, made from the reaction between sunlight and pollution, are showing up
in the western U.S. that have little or no industrial activity.
To what extent climate change due to the emission
of greenhouse gases may favor the formation
of an «
ozone hole»
in the Arctic
stratosphere is an important topic
of the POLSTRACC campaign.
And
ozone, which forms a beneficial shield against ultraviolet radiation when high
in the
stratosphere, is an efficient greenhouse gas when it appears at airliner altitudes — as it increasingly does, since it too is a by - product
of fossil fuel burning.
The Antarctic
ozone hole forms and expands during the Southern Hemisphere spring (August and September) because
of the high levels
of chemically active forms
of chlorine and bromine
in the
stratosphere.
They point out that the 50 per cent loss
of ozone at low altitudes
in the
stratosphere is equivalent to a 15 per cent loss
of total
ozone (Nature, vol 259, p 283).
On Earth, temperature inversion occurs because
ozone in the
stratosphere absorbs much
of the sun's ultraviolet radiation, preventing it from reaching the surface, protecting the biosphere, and therefore warming the
stratosphere instead.
They fear that similar aerosol already
in the northern
stratosphere, which came from the eruption
of Mount Pinatubo
in the Philippines
in June 1991, may cause a dramatic loss
of ozone in the northern hemisphere next February or March.
Scientists first detected the notorious «
ozone hole» over the South Pole 14 years ago, the apparent result
of chemical reactions caused by chlorofluorocarbons and other pollutants
in the
stratosphere.
On the basis
of its intended flight route, the Perlan glider might be able to provide the first direct observations
of polar stratospheric clouds, a unique type
of ice cloud that forms
in the polar
stratosphere and helps to deplete
ozone, Gong adds.
The temperature
of the
stratosphere is one
of the key factors
in the springtime depletion
of ozone above the Antarctic where
in winter it gets colder than anywhere else on Earth, encouraging icy particles to form
in polar stratospheric clouds.
For the first time, it has been shown that the rate
of ozone depletion
in the upper
stratosphere — 35 to 45 kilometres up — is slowing down.
Chlorine monoxide, which is produced by a similar series
of reactions involving icy particles
in the
stratosphere, is blamed for the springtime depletion
of ozone above Antarctica.
Rumen Bojkov,
of the UN's World Meteorological Organization, says this might explain the large losses
of ozone observed at lower altitudes
in the
stratosphere.
Air naturally poor
in ozone was, for example, lifted into the lower
stratosphere above Britain from the sub-tropical Atlantic, by an unusual pattern
of atmospheric circulation.
They find that even if
ozone - damaging chemicals (chiefly CFCs) are phased out
in line with current international agreements, the amount
of chlorine - bearing material
in the
stratosphere will continue to increase for several decades.
Every day, up to 500 civil aircraft
in the corridor burst out
of the troposphere and up into the
stratosphere, with its fragile
ozone layer.
Pollutants that gather from India and China
in the lowlands around the mountains can be boosted as high as 18 kilometers, reaching the
stratosphere — the atmospheric layer directly above the troposphere that contains most
of Earth's
ozone.
Unlike
ozone in the
stratosphere, which benefits life on Earth by blocking ultraviolet radiation from the Sun, ground - level
ozone can trigger a number
of health problems.
On Earth,
ozone absorbs UV
in the
stratosphere, protecting our world from a lot
of the Sun's harmful radiation.
A 20 - year study by German scientists has found that the rate
of increase
of CFC - 12, a chlorofluorocarbon compound that spawns
ozone - destroying reactions
in the
stratosphere, has slowed since 1990, although absolute levels are still rising.
And it could explain why past studies measured higher than expected levels
of ozone - damaging chemicals
in the
stratosphere, Rex says.
Because
ozone in the troposphere is a precursor to OH, they deployed weather balloons equipped with measuring devices known as sondes to measure the amount
of ozone in the air from the surface to the
stratosphere.
«This is the only long - term data set with regular measurements
of ozone - destroying compounds
in the
stratosphere,» says atmospheric chemist Darin Toohey
of the University
of California, Irvine.
Because they are released
in large quantities from tropical oceans, they are rapidly lofted by tropical thunderstorms into the
stratosphere within a month or two where they can destroy
ozone for a larger portion
of their lifetimes.
- Volcans do not add much
in the way
of ozone depleting chemicals into the
stratosphere.
Stratospheric cooling as a result
of excess CO2 does influence
ozone recovery, and
ozone changes
in the troposphere and
stratosphere to have effects on radiative balance
of the planet.
Temperature inversion
in Earth's
stratosphere occurs because
of the presence
of ozone, while on Jupiter and Saturn, it is caused by the presence
of hydrocarbons.
Polar stratospheric clouds (PSCs) are a sign
of extremely cold temperatures
in the
stratosphere and some types
of PSCs are responsible for
ozone destruction.
Today, high
in the
stratosphere, a thick layer
of ozone blankets the planet.
The chemical balance
in the
stratosphere is changed significantly by the presence
of these clouds, altering the breakdown products from manmade CFCs (chlorofluorocarbons) so that rapid chemical
ozone destruction can occur
in the presence
of sunlight.
No specific mention
of the «volume cold enough for
ozone loss» trend line is made
in the Nature text, although it is stated that «Certain clouds
in the
stratosphere provide surfaces on which CFC decay products are converted into forms that destroy
ozone â??
In the lower stratosphere — closest to the surface and close to the equator — increased CO2 is slowing the production of new ozone, especially in the sprin
In the lower
stratosphere — closest to the surface and close to the equator — increased CO2 is slowing the production
of new
ozone, especially
in the sprin
in the spring.
Higher levels
of carbon dioxide, however, do have an indirect effect on the
ozone layer
in the
stratosphere.