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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

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