Global stratospheric effects of the alumina emissions by
Global stratospheric effects of the alumina emissions by
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氧化铝排放对全球平流层的影响
DOI:
10.1029/2001jd900022
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发表时间:
2001
期刊:
影响因子:
--
通讯作者:
M. Prather
中科院分区:
文献类型:
--
作者:
M. Danilin;R. Shia;M. Ko;D. Weisenstein;N. Sze;J. J. Lamb;T. W. Smith;P. Lohn;M. Prather
We simulate accumulation of AleO3 particles in the atmosphere produced by solid-fueled rocket motors by using the Goddard Institute for Space Studies/University of California at Irvine three-dimensionM (3-D) chemistry- transport model (CTM). Our study differs from Jackman et al. (1998) by applying a 3-D CTM, considering 13 size bins for the emitted particles from 0.025 to 10/zm and taking into account their washout, gravitational sedimentation, and coagulation with background sulfate aerosol. We assume an initial trimodal size distribution of AleO3 particles (Beiting, 1997) with 2.8% by mass of the alumina emitted as particles with radius of less than i /zm. Our test case adopts a stratospheric source of 1120 tons/yr equivalent to nine space Shuttle and four Titan IV launches annually. The calculated steady state surface area density (SAD) and mass density for the scenarios with sedimentation of alumina particles have maximum values in the lower stratosphere in the Northern Hemisphere of up to 7x 10 -4 /zme/cm 3 and 0.09 ng/m 3, respectively, or about 1000 times smaller than those of the background sulfate aerosol. Our results are sensitive to the emitted mass fractionation of alumina (EMFA) showing the values for the SAD or mass density higher or lower by an order of magnitude owing to a poorly known EMFA. Chemical implications of alumina particle accumulation for the ozone balance are estimated by using the Atmospheric and Environmental Research 2-D model assuming chlorine activation on A1O3 surfaces vithe C1ONO + HC1 - CIq- HNO3 reaction withprobability of 0.02 (Molina et al., 1997). Owing to the very small AleO3 SAD, any additional ozone depletion due to AleO3 emissions is also small (0.0028% on a global annually averaged basis for the scenario with sedimentation, or about 4 times smaller than the ozone response to chlorine emissions only). The ozone depletion potential of the alumina emissions is about 0.03-0.08 for the scenarios using the EMFA of Beiting (1997) and larger by an order of magnitude for the EMFA of Brady and Martin (1995). weight), CO (24%), HC1 (21%), HO (10%), N2 (9%), CO2 (4%), and H2 (2%) emitted up to 42 km (Prather et al., 1990a). The environmental impact of the SRM emissions has been examined (e.g., World Meteorological Organization (WMO), 1992). It is believed that chlorine emissions (mostly in the form of HC1 and C12) pose the main risk for the ozone layer compared with the other SRM emissions. On the global scale, the depletion of the ozone column caused by SRM chlorine emissions is very small (<0.1% at northern midlatitudes and about 0.01% over the globe assuming nine space shuttle and six Titan IV launches annually) (Prather et al., 1990a;