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Vibrational and rotational cooling of electrons by water vaporThe cooling of electrons by vibrational and rotational excitation of water molecules plays an important role in the thermal balance of electrons in cometary ionospheres. The energy-loss function for rotational excitation and deexcitation of H2O by electron impact is calculated theoretically. The rotational cooling rate is calculated using this loss function for a wide range of electron and neutral temperatures. The vibrational cooling rate is calculated using measured values of electron-impact vibrational excitation cross sections. Analytical formulas are provided for some of the cooling rates. The interaction of ions with H2O molecules is also discussed, and a formula is suggested for the momentum-transfer collision frequency.
Document ID
19870037394
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Cravens, T. E.
(Michigan, University Ann Arbor, United States)
Korosmezey, A.
(Magyar Tudomanyos Akademia Kozponti Fizikai Kutato Intezet, Budapest, Hungary)
Date Acquired
August 13, 2013
Publication Date
October 1, 1986
Publication Information
Publication: Planetary and Space Science
Volume: 34
ISSN: 0032-0633
Subject Category
Astronomy
Accession Number
87A24668
Funding Number(s)
CONTRACT_GRANT: NAGW-15
CONTRACT_GRANT: NSF ATM-84-17884
CONTRACT_GRANT: NGR-23-005-015
Distribution Limits
Public
Copyright
Other

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