Manual for Refrigeration Servicing Technicians - UNEP - Division of ...
Manual for Refrigeration Servicing Technicians - UNEP - Division of ...
Manual for Refrigeration Servicing Technicians - UNEP - Division of ...
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1<br />
Environmental Impact<br />
1. The exosphere<br />
(2400km))<br />
The sunlight still contains very high-energy photons, which can heat gas<br />
particles in the exosphere up to 2,500 degrees C during the day.<br />
2. The ionosphere Most high energy photons are absorbed here leading to a few air<br />
molecules becoming electrically charged.<br />
3. The ozone layer This thin layer at the top <strong>of</strong> the stratosphere absorbs most <strong>of</strong> the ultraviolet<br />
(UV) light. Too much UV light can cause damage to living things<br />
so the ozone layer is very important in protecting life on Earth.<br />
4.The stratosphere<br />
(50km)<br />
5. The troposphere (8-15<br />
km).<br />
6. Absorption <strong>of</strong><br />
radiation emitted by the<br />
Earth<br />
Ozone depletion relies on the clouds in the stratosphere: Polar<br />
stratospheric clouds (PSCs), also known as nacreous clouds, are<br />
CLOUDS in the winter polar STRATOSPHERE at altitudes <strong>of</strong> 15,000–25,000<br />
metres (50,000–80,000 ft). They are implicated in the <strong>for</strong>mation <strong>of</strong> OZONE<br />
HOLES; [1] their effects on ozone depletion arise because they support<br />
chemical reactions.<br />
The troposphere contains most <strong>of</strong> the air molecules, nearly all the water<br />
vapour so all <strong>of</strong> the clouds are in this layer. All these particles mean that<br />
a lot <strong>of</strong> sunlight is scattered. Shorter wavelengths (violet and blue) are<br />
scattered more than longer wavelengths, making the sky appear blue.<br />
The Earth emits a lot <strong>of</strong> long wavelength radiation from its surface and<br />
much <strong>of</strong> this is absorbed and scattered in the troposphere. Greenhouse<br />
gases such as carbon dioxide and water vapour are responsible <strong>for</strong><br />
most <strong>of</strong> this absorption, making the temperature around the Earth<br />
higher.<br />
This ozone filter efficiently screens out almost<br />
all the harmful ultraviolet rays <strong>of</strong> the sun; the<br />
ozone layer absorbs most <strong>of</strong> the dangerous<br />
UV-B radiation (radiation between UV-A which<br />
is allowed through and UV-C which is mainly<br />
captured by oxygen, as indicated in Figure<br />
1.2). Any damage that is done to the ozone<br />
layer will lead to increased UV-B radiation.<br />
Increases <strong>of</strong> UV-B radiation have been clearly<br />
observed in areas experiencing periods <strong>of</strong><br />
intense ozone depletion.<br />
Any increased UV-B that reaches the earth’s<br />
surface has a potential to cause considerable<br />
harm to the environment and to life on earth.<br />
A small decrease in the ozone layer could<br />
significantly increase the incidence <strong>of</strong> skin<br />
cancer, and could lead to an acceleration<br />
<strong>of</strong> the rarer but more virulent <strong>for</strong>m <strong>of</strong><br />
cancer known as coetaneous malignant<br />
melanoma. Increased UV-B could lead to<br />
increased incidents <strong>of</strong> eye damage, including<br />
cataracts, de<strong>for</strong>mation <strong>of</strong> the eye lenses, and<br />
presbyopia. Eye cataracts, the leading cause<br />
<strong>of</strong> blindness in the world, are expected to<br />
increase considerably.<br />
18