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Fractionation of hydrogen and deuterium on Venus due to collisional ejectionThe collisional ejection process for hydrogen on Venus is reanalyzed. Improved values for the efficiency of H and D escape as a function of the ionospheric temperature are reported. It is proposed that the reduction of the hydrogen flux for collisional ejection be reduced from 8 to 3.5 x 10 exp 6/sq cm/s, and a revised D/H fractional factor of 0.47 due to collisional ejection is suggested. The resulting deuterium flux is 3.1 x 10 exp 4/sq cm/s, roughly six times the flux due to charge exchange, making collisional ejection the dominant escape mechanism for deuterium on Venus.
Document ID
19930053304
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Gurwell, Mark A.
(NASA Ames Research Center Moffett Field, CA, United States)
Yung, Yuk L.
(California Inst. of Technology Pasadena, United States)
Date Acquired
August 16, 2013
Publication Date
February 1, 1993
Publication Information
Publication: Planetary and Space Science
Volume: 41
Issue: 2
ISSN: 0032-0633
Subject Category
Lunar And Planetary Exploration
Accession Number
93A37301
Funding Number(s)
CONTRACT_GRANT: NAG2-764
Distribution Limits
Public
Copyright
Other

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