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Models of Venus neutral upper atmosphere - Structure and compositionModels of the Venus neutral upper atmosphere, based on both in situ and remote sensing measurements, are provided for the height interval from 100 to 3500 km. The general approach in model formulation was to divide the atmosphere into three regions: 100-150 km, 150-250 km, and 250-3500 km. Boundary conditions at 150 km are consistent with both drag and mass spectrometer measurements. A paramount consideration was to keep the models simple enough to be used conveniently. Available observations are reviewed.
Document ID
19870027598
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1016/0273-1177(85)90200-5
Authors
Keating, G. M. (NASA Langley Research Center Hampton, VA, United States)
Bertaux, J. L. (CNRS Service d'Aeronomie, Verrieres-le-Buisson, France)
Bougher, S. W. (NASA Langley Research Center Hampton, VA, United States)
Dickinson, R. E. (National Center for Atmospheric Research Boulder, CO, United States)
Cravens, T. E. (Michigan, University Ann Arbor, United States)
Hedin, A. E. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 13, 2013
Publication Date
January 1, 1985
Publication Information
Publication: Advances in Space Research
Volume: 5
Issue: 11, 1
ISSN: 0273-1177
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
ISSN: 0273-1177
Accession Number
87A14872
Distribution Limits
Public
Copyright
Other

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