Improved representation of the global dust cycle using observational constraints on dust properties and abundance
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Published:2021-05-27
Issue:10
Volume:21
Page:8127-8167
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ISSN:1680-7324
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Container-title:Atmospheric Chemistry and Physics
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language:en
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Short-container-title:Atmos. Chem. Phys.
Author:
Kok Jasper F.ORCID, Adebiyi Adeyemi A., Albani SamuelORCID, Balkanski YvesORCID, Checa-Garcia RamiroORCID, Chin Mian, Colarco Peter R.ORCID, Hamilton Douglas S.ORCID, Huang YueORCID, Ito AkinoriORCID, Klose MartinaORCID, Leung Danny M.ORCID, Li Longlei, Mahowald Natalie M., Miller Ron L.ORCID, Obiso Vincenzo, Pérez García-Pando CarlosORCID, Rocha-Lima Adriana, Wan Jessica S.ORCID, Whicker Chloe A.
Abstract
Abstract. Even though desert dust is the most abundant aerosol by
mass in Earth's atmosphere, atmospheric models struggle to accurately
represent its spatial and temporal distribution. These model errors are
partially caused by fundamental difficulties in simulating dust emission in
coarse-resolution models and in accurately representing dust microphysical
properties. Here we mitigate these problems by developing a new methodology
that yields an improved representation of the global dust cycle. We present
an analytical framework that uses inverse modeling to integrate an ensemble
of global model simulations with observational constraints on the dust size
distribution, extinction efficiency, and regional dust aerosol optical
depth. We then compare the inverse model results against independent
measurements of dust surface concentration and deposition flux and find that
errors are reduced by approximately a factor of 2 relative to current
model simulations of the Northern Hemisphere dust cycle. The inverse model
results show smaller improvements in the less dusty Southern Hemisphere,
most likely because both the model simulations and the observational
constraints used in the inverse model are less accurate. On a global basis,
we find that the emission flux of dust with a geometric diameter up to 20 µm (PM20) is approximately 5000 Tg yr−1, which is greater than most
models account for. This larger PM20 dust flux is needed to match
observational constraints showing a large atmospheric loading of coarse
dust. We obtain gridded datasets of dust emission, vertically integrated
loading, dust aerosol optical depth, (surface) concentration, and wet and
dry deposition fluxes that are resolved by season and particle size. As our
results indicate that this dataset is more accurate than current model
simulations and the MERRA-2 dust reanalysis product, it can be used to
improve quantifications of dust impacts on the Earth system.
Funder
National Science Foundation Army Research Office Office of the President, University of California European Commission Japan Society for the Promotion of Science Ministero dell’Istruzione, dell’Università e della Ricerca AXA Research Fund Ministerio de Ciencia e Innovación
Publisher
Copernicus GmbH
Subject
Atmospheric Science
Reference187 articles.
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