Eddy evolution during large dust storms

The evolution of eddy kinetic energy during the development of large regional dust storms on Mars is investigated using the Mars Analysis Correction Data Assimilation (MACDA) reanalysis product and the dust storm data derived from Mars Global Surveyor Mars Daily Global Maps. Transient eddies in MACD...

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Bibliographic Details
Published in:Icarus (New York, N.Y. 1962) N.Y. 1962), 2020-03, Vol.338, p.113507, Article 113507
Main Authors: Battalio, Michael, Wang, Huiqun
Format: Article
Language:English
Subjects:
Atmospheres, Dynamics
Mars, Atmosphere
Mars, Climate
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Summary:The evolution of eddy kinetic energy during the development of large regional dust storms on Mars is investigated using the Mars Analysis Correction Data Assimilation (MACDA) reanalysis product and the dust storm data derived from Mars Global Surveyor Mars Daily Global Maps. Transient eddies in MACDA are decomposed into different components according to their eddy periods: P≤1 sol, 1
ISSN:0019-1035
1090-2643
DOI:10.1016/j.icarus.2019.113507