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Equatorial gyroresonance between electrons and magnetospherically reflected whistlersMagnetospherically reflected whistlers resonantly interact with energetic (of order 100 keV) electrons in a relatively narrow energy range during multiple equatorial crossings over a wide range of L-shells (L between 1.5 and 4). Results indicate that wave energy that enters the magnetosphere at a fixed location can potentially contribute to the loss of particles over a wide range of latitudes.
Document ID
19910026443
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Jasna, D.
(Stanford Univ. CA, United States)
Inan, U. S.
(Stanford Univ. CA, United States)
Bell, T. F.
(Stanford University CA, United States)
Date Acquired
August 14, 2013
Publication Date
October 1, 1990
Publication Information
Publication: Geophysical Research Letters
Volume: 17
ISSN: 0094-8276
Subject Category
Geophysics
Accession Number
91A11066
Funding Number(s)
CONTRACT_GRANT: NAGW-1582
Distribution Limits
Public
Copyright
Other

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