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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 />

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

Table of contents | Previous page | Next page<br />

5.3. Detectability of Changes in Ground-Level Irradiance<br />

Our ability to detect future changes in solar UV irradiance attributable to increases in aircraft<br />

emissions depends on two factors. The first factor is <strong>the</strong> size of <strong>the</strong> expected change relative to<br />

natural variability <strong>and</strong> long-term changes from o<strong>the</strong>r human causes. The second factor is <strong>the</strong><br />

accuracy <strong>and</strong> stability with which we are capable of making measurements over long periods of time.<br />

The detection of a long-term change in UVery depends on <strong>the</strong> size of <strong>the</strong> expected change, <strong>the</strong><br />

length of <strong>the</strong> data record over which <strong>the</strong> change occurs, <strong>and</strong> <strong>the</strong> variability of UVery. Wea<strong>the</strong>rhead et<br />

al. (1998) show that a data record of at least 15 years is necessary to distinguish a statistically<br />

significant (2-sigma) long-term change of 5% per decade in UVery from <strong>the</strong> natural variability present<br />

at most sites. A long-term change of 5% over 50 years (1% per decade to 2050) would just be<br />

detectable at <strong>the</strong> best sites. The o<strong>the</strong>r factor is whe<strong>the</strong>r existing instrumentation is able to detect<br />

expected long-term changes. Presently, many different instruments devoted to monitoring changes in<br />

solar UV during forthcoming decades are deployed over <strong>the</strong> globe. These instruments are ei<strong>the</strong>r<br />

spectroradiometers or broadb<strong>and</strong> <strong>and</strong> narrowb<strong>and</strong> detectors operating in <strong>the</strong> UV region.<br />

Spectroradiometers are <strong>the</strong> most suitable instruments because <strong>the</strong>y provide detailed measurements<br />

of global spectral irradiance, which can be used to assess <strong>the</strong> importance of various UV-controlling<br />

factors. Because of <strong>the</strong> weak intensity of UV irradiance relative to o<strong>the</strong>r parts of <strong>the</strong> solar spectrum,<br />

however, it is only in recent years that <strong>the</strong> quality of such measurements has become sufficient to<br />

detect interannual changes in UV irradiance that are attributable to year-to-year changes in ozone<br />

over relatively short (< 10 years) measurement records (Kerr <strong>and</strong> McElroy, 1993; McKenzie et al.,<br />

1993; Kerr <strong>and</strong> McElroy, 1994; Gardiner <strong>and</strong> Kirsch, 1995; Groebner et al., 1996; Bais et al., 1997;<br />

Gurney, 1998). The quality of o<strong>the</strong>r types of broadb<strong>and</strong> instruments cannot yet be considered<br />

sufficient to detect <strong>the</strong>se small long-term UV changes (Leszczynski et al., 1996; Mayer <strong>and</strong><br />

Seckmeyer, 1996; Blumthaler, 1997; Wea<strong>the</strong>rhead et al., 1997; WMO, 1997).<br />

http://www.ipcc.ch/ipccreports/sres/aviation/058.htm (1 von 3)08.05.2008 02:42:39<br />

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