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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 />

3.3.5. Soot<br />

O<strong>the</strong>r reports in this collection<br />

The primary atmospheric source of soot or black carbon particles is combustion of fossil fuels <strong>and</strong> biomass burning at <strong>the</strong> Earth's surface, with total emission values<br />

near 12 Tg C yr -1 (Liousse et al., 1996). This value exceeds reasonable estimates of <strong>the</strong> aircraft source of black carbon by several orders of magnitude (Bekki, 1997).<br />

For example, aircraft are estimated to have emitted 0.0015 to 0.015 Tg C as soot into <strong>the</strong> atmosphere in 1992 [with EI(soot) of 0.01 to 0.1 g C/kg fuel] (Friedl, 1997;<br />

Rahmes et al., 1998). As in <strong>the</strong> case of sulfate aerosol, deposition <strong>and</strong> scavenging of black carbon near surface sources creates large vertical gradients in <strong>the</strong> lower<br />

atmosphere, with soot concentrations falling by 1 to 2 orders of magnitude between <strong>the</strong> surface <strong>and</strong> <strong>the</strong> lower stratosphere (Penner et al., 1992; Cooke <strong>and</strong> Wilson,<br />

1996; Liousse et al., 1996). A possible meteoritic source of soot in <strong>the</strong> lower stratosphere has been considered but is not well quantified at present (Chuan <strong>and</strong> Woods,<br />

1984).<br />

Few direct measurements of soot abundance are available in <strong>the</strong> upper troposphere <strong>and</strong><br />

lower stratosphere. The most extensive measurements in <strong>the</strong>se regions are from aircraft<br />

impactor measurements (Pueschel et al., 1992, 1997; Blake <strong>and</strong> Kato, 1995). The accuracy<br />

of such measurements depends on knowledge of <strong>the</strong> impactor for small soot particles. The<br />

results (Figure 3-10) are considered to represent a lower limit for soot number <strong>and</strong> mass<br />

because of size-selective sampling <strong>and</strong> because of scavenging of soot by background<br />

aerosol particles. Features of <strong>the</strong> measurements include a large gradient between <strong>the</strong><br />

Nor<strong>the</strong>rn <strong>and</strong> Sou<strong>the</strong>rn Hemispheres <strong>and</strong> large variability with altitude at nor<strong>the</strong>rn midlatitudes.<br />

The large vertical variability of soot at nor<strong>the</strong>rn mid-latitudes cannot be explained<br />

by <strong>the</strong> accumulation of aircraft soot emissions. With typical soot mass densities observed to<br />

be approximately 1 ng m -3 , soot is estimated to represent approximately 0.01% of <strong>the</strong><br />

stratospheric aerosol mass (Pueschel et al., 1992). In o<strong>the</strong>r sampling flights over sou<strong>the</strong>rn<br />

Germany, measurements of absorbing mass (probably soot) at 8-12 km altitude <strong>and</strong> partly<br />

within cirrus clouds showed concentrations above 10 ng m -3 , with higher values correlated<br />

with local aviation fuel consumption (Ström <strong>and</strong> Ohlsson, 1998).<br />

http://www.ipcc.ch/ipccreports/sres/aviation/037.htm (1 von 3)08.05.2008 02:42:02

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