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New fine structure cooling rateOne of the dominant electron cooling processes in the ionosphere is caused by electron impact induced fine structure transitions among the ground state levels of atomic oxygen. This fine structure cooling rate is based on theoretical cross sections. Recent advances in the numerical cross section determinations to include polarization effects and more accurate representations of the atomic target result in new lower values. These cross sections are employed in this paper to derive a new fine structure cooling rate which is between 40% and 60% of the currently used rate. A new generalized formula is presented for the cooling rate (from which the fine structure cooling rate is derived), valid for arbitrary mass and temperature difference of the colliding particles and arbitrary inelastic energy difference.
Document ID
19760062492
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Hoegy, W. R.
(NASA Goddard Space Flight Center Greenbelt, Md., United States)
Date Acquired
August 8, 2013
Publication Date
September 1, 1976
Publication Information
Publication: Geophysical Research Letters
Volume: 3
Subject Category
Geophysics
Accession Number
76A45458
Distribution Limits
Public
Copyright
Other

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