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Static stability and thermal wind in an atmosphere of variable composition Applications to MarsRadiometric measurements of the temperature of the south polar cap of Mars in winter have yielded values significantly below the expected 148 K. One proposed explanation for this result is a substantial reduction in the CO2 content of the atmosphere and a lowering of the mean molecule weight near the surface. The meteorological consequences of this explanation are explored by deriving a criterion for vertical static stability and a thermal wind law for an atmosphere of variable composition. The atmosphere proves to be statically unstable unless the anomaly in the CO2 mixing ratio extends to heights of tens of kilometers. The effect of varying molecular weight exceeds the effect of temperature gradient, producing shears with height of reversed sign. The shears are baroclinically unstable, and this instability would eradicate the latitudinal gradient of molecular weight. This inconsistency can be resolved by invoking a reasonable elevation of the central polar cap and by imposing an adequate zonal wind. It is concluded that if the explanation requiring a change in atmospheric composition is correct, it must be accompanied by other special circumstances to make it meteorologically consistent.
Document ID
19790056629
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Hess, S. L.
(Florida State University Tallahassee, Fla., United States)
Date Acquired
August 9, 2013
Publication Date
June 10, 1979
Publication Information
Publication: Journal of Geophysical Research
Volume: 84
Subject Category
Lunar And Planetary Exploration
Accession Number
79A40642
Funding Number(s)
CONTRACT_GRANT: NAS1-9693
Distribution Limits
Public
Copyright
Other

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