Mineral dust aerosols in the NASA goddard institute for Space Sciences ModelE atmospheric general circulation model

被引:160
作者
Miller, RL
Cakmur, RV
Perlwitz, J
Geogdzhayev, IV
Ginoux, P
Koch, D
Kohfeld, KE
Prigent, C
Ruedy, R
Schmidt, GA
Tegen, I
机构
[1] Columbia Univ, Dept Appl Phys & Appl Math, New York, NY 10025 USA
[2] NASA, Goddard Inst Space Studies, New York, NY 10025 USA
[3] Natl Acad Sci, Washington, DC 20418 USA
[4] NOAA, Geophys Fluid Dynam Lab, Princeton, NJ 08542 USA
[5] Columbia Univ, Ctr Climate Syst Res, New York, NY USA
[6] CUNY Queens Coll, Sch Earth & Environm Sci, Flushing, NY 11367 USA
[7] Observ Paris, CNRS, Lab Etud Rayonnement & Mat Astrophys, F-75014 Paris, France
[8] Leibniz Inst Tropospher Res, D-04318 Leipzig, Germany
关键词
D O I
10.1029/2005JD005796
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
We describe an updated model of the dust aerosol cycle embedded within the NASA Goddard Institute for Space Studies 'ModelE' atmospheric general circulation model (AGCM). The model dust distribution is compared to observations ranging from aerosol optical thickness and surface concentration to deposition and size distribution. The agreement with observations is improved compared to previous distributions computed by either an older version of the GISS AGCM or an offline tracer transport model. The largest improvement is in dust transport over the Atlantic due to increased emission over the Sahara. This increase comes from subgrid wind fluctuations associated with dry convective eddies driven by intense summertime heating. Representation of 'preferred sources' of soil dust particles is also fundamental to the improvement. The observations suggest that deposition is too efficient in the model, partly due to AGCM rainfall errors.
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页数:19
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