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Magnetospheric filter effect for Pc 3 Alfven mode wavesWe present a ray-tracing study of the propagation of Pc 3 Alfven mode waves originating at the dayside magnetopause. This study reveals interesting features of magnetospheric filter effect for these waves. Pc 3 Alfven mode waves cannot penetrate to low Earth altitudes unless the wave frequency is below approximately 30 mHz. Configurations of the dispersion curves and the refractive index show that the gyroresonance and pseudo-cutoff introduced by the heavy ion O(+) block the waves. When the O(+) concentration is removed from the plasma composition, the barriers caused by the O(+) no longer exist, and waves with much higher frequencies than 30 mHz can penetrate to low altitudes. The result that the 30 mHz or lower frequency Alfven waves can be guided to low altitudes agrees with ground-based power spectrum observation at high altitudes.
Document ID
19960014066
Acquisition Source
Headquarters
Document Type
Reprint (Version printed in journal)
Authors
Zhang, X.
(Alabama Univ. Huntsville, AL United States)
Comfort, R. H.
(Alabama Univ. Huntsville, AL United States)
Gallagher, D. L.
(NASA Marshall Space Flight Center Huntsville, AL United States)
Green, J. L.
(NASA Goddard Space Flight Center Greenbelt, MD United States)
Musielak, Z. E.
(Alabama Univ. Huntsville, AL United States)
Moore, T. E.
(NASA Marshall Space Flight Center Huntsville, AL United States)
Date Acquired
September 6, 2013
Publication Date
June 1, 1995
Subject Category
Geophysics
Report/Patent Number
NASA-CR-199998
Paper 95JA00276
NAS 1.26:199998
Report Number: NASA-CR-199998
Report Number: Paper 95JA00276
Report Number: NAS 1.26:199998
Accession Number
96N19526
Funding Number(s)
CONTRACT_GRANT: NAGw-1630
PROJECT: RTOP 432-20-00
CONTRACT_GRANT: NAG8-239
CONTRACT_GRANT: NSF ATM-91-19580
Distribution Limits
Public
Copyright
Public Use Permitted.
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