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Assimilating and Modeling Dust Transport in the Martian Climate System

Published online by Cambridge University Press:  29 April 2014

Tao Ruan ,
Luca Montabone ,
Peter L. Read  and
Stephen R. Lewis
Tao Ruan
Affiliation:
Atmospheric, Oceanic & Planetary Physics, University of Oxford, Oxford, OX1 3PU, United Kingdom email: [email protected]
Luca Montabone
Affiliation:
Atmospheric, Oceanic & Planetary Physics, University of Oxford, Oxford, OX1 3PU, United Kingdom email: [email protected] Université Pierre et Marie Curie, Laboratoire de Météorologie Synamique, Paris, France email: [email protected]
Peter L. Read
Affiliation:
Atmospheric, Oceanic & Planetary Physics, University of Oxford, Oxford, OX1 3PU, United Kingdom email: [email protected]
Stephen R. Lewis
Affiliation:
Dept. of Physical Sciences, & The Open University, Walton Hall, Milton Keynes, MK7 6AA, United Kingdom email: [email protected]
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Abstract

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A meteorological data assimilation system has been developed recently for analyzing measurements of temperature and dust opacity on Mars and has been successfully applied in several studies (e.g. Montabone et al. 2005, Lewis et al. 2007) to study various atmospheric phenomena. A more sophisticated data assimilation system, now with full dust transport incorporated, is becoming available to represent more accurately and realistically the physical transport of dust.

Keywords

hydrodynamicsplanets and satellites: generalmethods: data analysismethods: numerical
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S293: Formation, Detection, and Characterization of Extrasolar Habitable Planets , August 2012 , pp. 326 - 328
Copyright
Copyright © International Astronomical Union 2014 

References

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