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How the Assumed Size Distribution of Dust Minerals Affects the Predicted Ice Forming NucleiThe formation of ice in clouds depends on the availability of ice forming nuclei (IFN). Dust aerosol particles are considered the most important source of IFN at a global scale. Recent laboratory studies have demonstrated that the mineral feldspar provides the most efficient dust IFN for immersion freezing and together with kaolinite for deposition ice nucleation, and that the phyllosilicates illite and montmorillonite (a member of the smectite group) are of secondary importance.A few studies have applied global models that simulate mineral specific dust to predict the number and geographical distribution of IFN. These studies have been based on the simple assumption that the mineral composition of soil as provided in data sets from the literature translates directly into the mineral composition of the dust aerosols. However, these tables are based on measurements of wet-sieved soil where dust aggregates are destroyed to a large degree. In consequence, the size distribution of dust is shifted to smaller sizes, and phyllosilicates like illite, kaolinite, and smectite are only found in the size range 2 m. In contrast, in measurements of the mineral composition of dust aerosols, the largest mass fraction of these phyllosilicates is found in the size range 2 m as part of dust aggregates. Conversely, the mass fraction of feldspar is smaller in this size range, varying with the geographical location. This may have a significant effect on the predicted IFN number and its geographical distribution.An improved mineral specific dust aerosol module has been recently implemented in the NASA GISS Earth System ModelE2. The dust module takes into consideration the disaggregated state of wet-sieved soil, on which the tables of soil mineral fractions are based. To simulate the atmospheric cycle of the minerals, the mass size distribution of each mineral in aggregates that are emitted from undispersed parent soil is reconstructed. In the current study, we test the null-hypothesis that simulating the presence of a large mass fraction of phyllosilicates in dust aerosols in the size range 2 m, in comparison to a simple model assumption where this is neglected, does not yield a significant effect on the magnitude and geographical distribution of the predicted IFN number. Results from sensitivity experiments are presented as well.
Document ID
20160000369
Acquisition Source
Goddard Space Flight Center
Document Type
Presentation
Authors
Perlwitz, Jan P.
(Columbia Univ. New York, NY, United States)
Fridlind, Ann M.
(NASA Goddard Inst. for Space Studies New York, NY United States)
Garcia-Pando, Carlos Perez
(Columbia Univ. New York, NY, United States)
Miller, Ron L.
(NASA Goddard Inst. for Space Studies New York, NY United States)
Knopf, Daniel A.
(Stony Brook Univ. Stony Brook, NY, United States)
Date Acquired
January 6, 2016
Publication Date
December 14, 2015
Subject Category
Meteorology And Climatology
Report/Patent Number
GSFC-E-DAA-TN28642
Meeting Information
Meeting: AGU Fall Meeting
Location: San Francisco, CA
Country: United States
Start Date: December 14, 2015
End Date: December 18, 2015
Sponsors: American Geophysical Union
Funding Number(s)
CONTRACT_GRANT: NNX14AB99A
Distribution Limits
Public
Copyright
Public Use Permitted.
Keywords
Dust
Size distribution
Minerals
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