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On empirical models of the upper atmosphere in the polar regions.The expression for the exospheric temperature in Jacchia's static diffusion models of the upper atmosphere has a discontinuous gradient at the poles. Therefore it cannot describe the true state of the upper atmosphere in the polar regions. Furthermore, it cannot be used to calculate quantities that depend on the derivative of the exospheric temperature, or the density, like pressure gradients, horizontal forces or horizontal heat fluxes. A modified expression for the exospheric temperature is suggested. This modification yields variables of state of the upper atmosphere that deviate little from Jacchia's values, but it has continuous gradient at the poles and is therefore more suitable for treating dynamical problems like the global wind pattern.
Document ID
19730041113
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Blum, P. W.
Harris, I.
(NASA Goddard Space Flight Center Greenbelt, Md., United States)
Date Acquired
August 7, 2013
Publication Date
March 1, 1973
Publication Information
Publication: Planetary and Space Science
Volume: 21
Subject Category
Geophysics
Accession Number
73A25915
Distribution Limits
Public
Copyright
Other

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