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The influence of convection electric fields on thermal proton outflow from the ionosphereThe continuity, momentum and energy hydrodynamic equations for an O(+)-H(+) ionosphere have been solved self-consistently for steady state conditions when a perpendicular (convection) electric field is present. Comparison of the H(+) temperature profiles obtained with and without the electric field show that the effect of the electric field is to enhance the H(+) temperature at high altitudes from about 3600 to 6400 K. Due to ion heating by the electric field, there is a net reduction of O(+) in the F2-region as compared with the case of a nonconvecting ionosphere. When the reduction of O(+) is neglected, the electric field acts to increase the H(+) outward flux. However, when the reduction of O(+) is included, there is a net reduction in the outward H(+) flux. Nevertheless, the convection electric field still results in an increase in the rate of depletion of the F-region ionization due to H(+) outflow, by a factor of 2.2 for a 100 mV/m electric field.
Document ID
19770050741
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Raitt, W. J.
(California, University La Jolla, Calif.; London, University College, Dorking, Surrey, United Kingdom)
Schunk, R. W.
(California Univ. La Jolla, CA, United States)
Banks, P. M.
(California, University La Jolla, Calif., United States)
Date Acquired
August 9, 2013
Publication Date
March 1, 1977
Publication Information
Publication: Planetary and Space Science
Volume: 25
Subject Category
Geophysics
Accession Number
77A33593
Funding Number(s)
CONTRACT_GRANT: NGR-05-009-075
CONTRACT_GRANT: NSF DES-74-22343
Distribution Limits
Public
Copyright
Other

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