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A model of a Martian Great dust storm.The great Martian 1971 dust storm is described using Carrier's (1971) model of a terrestrial hurricane with a somewhat modified thermodynamic drive. The model predicts the course of development and the time elapsing in three different phases: growth, maturity, decay. All the predictions correspond reasonably well to the observed phenomena. Explanations are offered for the rarity of the storms and the time of year and location at which they most commonly commence.
Document ID
19730040913
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Gierasch, P. J.
Goody, R. M.
(Harvard University Cambridge, Mass., United States)
Date Acquired
August 7, 2013
Publication Date
March 1, 1973
Publication Information
Publication: Journal of the Atmospheric Sciences
Volume: 30
Subject Category
Space Sciences
Accession Number
73A25715
Funding Number(s)
CONTRACT_GRANT: NSF GA-33990X
CONTRACT_GRANT: NAS1-9693
CONTRACT_GRANT: NSF GA-37012
Distribution Limits
Public
Copyright
Other

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