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Aviation and the Global Atmosphere

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<strong>Aviation</strong> <strong>and</strong> <strong>the</strong> <strong>Global</strong> <strong>Atmosphere</strong><br />

economic <strong>and</strong> technological assumptions, estimate a rise in global mean temperature of 1-3.5°C (best estimate 2°C) between 1990 <strong>and</strong> 2100. In all cases,<br />

<strong>the</strong> average rate of warming would probably be greater than any in <strong>the</strong> past 10,000 years, though actual annual-to-decadal changes would include<br />

considerable natural variability. A general warming is expected to lead to an increase in <strong>the</strong> occurrence of extremely hot days <strong>and</strong> a decrease in <strong>the</strong><br />

occurrence of extremely cold days. Regional temperature changes could differ substantially from <strong>the</strong> global mean value, <strong>and</strong> <strong>the</strong>re are many uncertainties<br />

about <strong>the</strong> scale <strong>and</strong> impacts of climate change, particularly at <strong>the</strong> regional level. The mean sea level is expected to rise 15-95 cm (best estimate 50 cm) by<br />

2100, with some flooding of low-lying areas. Forests, deserts, rangel<strong>and</strong>s, <strong>and</strong> o<strong>the</strong>r unmanaged ecosystems would face new climatic stresses, partly as a<br />

result of changes in <strong>the</strong> hydrological cycle; many could decline or fragment, with some individual species of flora or fauna becoming extinct. Because of <strong>the</strong><br />

delaying effect of <strong>the</strong> oceans, surface temperatures do not respond immediately to greenhouse gas emissions, so climate change would continue for many<br />

decades even if atmospheric concentrations were stabilized.<br />

Achieving stabilized atmospheric concentrations of greenhouse gases would dem<strong>and</strong> a major effort. For CO2 alone, freezing global emissions at <strong>the</strong>ir current<br />

rates would result in a doubling of its atmospheric concentrations from pre-industrial levels soon after 2100. Eventually, emissions would have to decrease<br />

well below current levels for concentrations to stabilize at doubled CO2 levels, <strong>and</strong> <strong>the</strong>y would have to continue to fall <strong>the</strong>reafter to maintain a constant CO2 concentration. The radiative forcing of greenhouse gas levels (including methane, nitrous oxide, <strong>and</strong> o<strong>the</strong>rs, but not aerosols) could equal that caused by a<br />

doubling of pre-industrial CO2 concentrations by 2030 <strong>and</strong> a trebling or more by 2100.<br />

The international community is tackling this challenge through <strong>the</strong> United Nations Framework Convention on Climate Change (UNFCCC). Adopted in 1992,<br />

<strong>the</strong> Convention seeks to stabilize atmospheric concentrations of greenhouse gases at safe levels. More than 170 countries have become Parties to <strong>the</strong><br />

Convention. Developed countries have agreed to take voluntary measures aimed at returning <strong>the</strong>ir emissions to 1990 levels by <strong>the</strong> year 2000, with fur<strong>the</strong>r<br />

legally binding emissions cuts after <strong>the</strong> year 2000 proposed at Kyoto in late 1997. Developed countries have also agreed to promote financial <strong>and</strong><br />

technological transfers to developing countries to help <strong>the</strong>m address climate change.<br />

Source: IPCC, 1996a.<br />

Box 1-2. Stratospheric Ozone Depletion, UV-B Radiation, <strong>and</strong> <strong>the</strong> Montreal Protocol<br />

Although ozone can be measured throughout much of <strong>the</strong> atmosphere, most of it is found in <strong>the</strong> stratosphere in a layer centered about 20 km above <strong>the</strong><br />

Earth's surface. Stratospheric ozone is beneficial to life on Earth because it blocks much of <strong>the</strong> dangerous ultraviolet light (UV-B) radiated by <strong>the</strong> sun. If<br />

unnaturally high levels of UV-B radiation reach <strong>the</strong> Earth's surface, many forms of life can be harmed. For instance, UV-B can cause skin cancers in humans<br />

<strong>and</strong> may reduce crop yields.<br />

Natural ozone amounts in <strong>the</strong> stratosphere result from a balance of production <strong>and</strong> loss processes involving chemistry, meteorology, <strong>and</strong> solar radiation.<br />

Since <strong>the</strong> 1960s, however, increases in atmospheric concentrations of human-generated chlorine- <strong>and</strong> bromine-containing compounds (principally<br />

chlorofluorocarbons <strong>and</strong> halons) have caused additional ozone loss. This trend has resulted in declines in stratospheric ozone amounts at middle <strong>and</strong> high<br />

latitudes in both hemispheres. The most dramatic manifestation is <strong>the</strong> Antarctic ozone hole, where more than half of <strong>the</strong> ozone is destroyed in a 6-week<br />

period each spring. In recent winters, similar features-but with half <strong>the</strong> ozone loss (20-30%)-have been observed over <strong>the</strong> Arctic, <strong>and</strong> at nor<strong>the</strong>rn midlatitudes<br />

a long-term decline of 5-10% has occurred over <strong>the</strong> past 20-30 years. Annual amounts of biologically active UV-B radiation have increased by about<br />

10% over mid-latitudes since 1979. No significant loss of ozone or increase in UV-B radiation has been found in <strong>the</strong> tropics.<br />

http://www.ipcc.ch/ipccreports/sres/aviation/014.htm (2 von 4)08.05.2008 02:41:26

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