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Titel |
Dust emission size distribution impact on aerosol budget and radiative forcing over the Mediterranean region: a regional climate model approach |
VerfasserIn |
P. Nabat, F. Solmon, M. Mallet, J. F. Kok, S. Somot |
Medientyp |
Artikel
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Sprache |
Englisch
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ISSN |
1680-7316
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Digitales Dokument |
URL |
Erschienen |
In: Atmospheric Chemistry and Physics ; 12, no. 21 ; Nr. 12, no. 21 (2012-11-12), S.10545-10567 |
Datensatznummer |
250011582
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Publikation (Nr.) |
copernicus.org/acp-12-10545-2012.pdf |
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Zusammenfassung |
The present study investigates the dust emission and load over the
Mediterranean basin using the coupled chemistry–aerosol–regional climate
model RegCM-4. The first step of this work focuses on dust particle emission
size distribution modeling. We compare a parameterization in which the
emission is based on the individual kinetic energy of the aggregates striking
the surface to a recent parameterization based on an analogy with the
fragmentation of brittle materials. The main difference between the two dust
schemes concerns the mass proportion of fine aerosol that is reduced in the
case of the new dust parameterization, with consequences for optical
properties. At the episodic scale, comparisons between RegCM-4 simulations,
satellite and ground-based data show a clear improvement using the new dust
distribution in terms of aerosol optical depth (AOD) values and geographic
gradients. These results are confirmed at the seasonal scale for the
investigated year 2008. This change of dust distribution has sensitive
impacts on the simulated regional dust budget, notably dry dust deposition
and the regional direct aerosol radiative forcing over the Mediterranean
basin. In particular, we find that the new size distribution produces a
higher dust deposition flux, and smaller top of atmosphere (TOA) dust
radiative cooling. A multi-annual simulation is finally carried out using the
new dust distribution over the period 2000–2009. The average SW radiative
forcing over the Mediterranean Sea reaches −13.6 W m−2 at the
surface, and −5.5 W m−2 at TOA. The LW radiative forcing is positive
over the basin: 1.7 W m−2 on average over the Mediterranean Sea at the
surface, and 0.6 W m−2 at TOA. |
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