NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
The propagation of low-frequency whistler waves driven by ion beams in the magnetotailThe generation and propagation of low-frequency whistler waves excited by ion beams in the plasma sheet boundary layer are followed using standard ray tracing techniques and assuming a Harris-type neutral sheet magnetic field profiles. The density is chosen such that the total pressure remains constant. The wave energy is calculated along the wave path taking into account growth due to the ion beam while the wave is in the plasma sheet boundary layer as well as damping due to resonant interactions with the background plasma. The results show that the electromagnetic waves are guided toward the central plasma sheet by the plasma gradients but are damped out before reaching the neutral plane itself due to Cerenkov resonance with the hot central plasma sheet background ions. The amplitudes and final positions of the waves depend on the temperature of the background plasma, the ion beam drift speed, and the ion beam thermal speed.
Document ID
19930039179
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Burinskaia, T.
(Russian Academy of Sciences, Space Research Inst. Moscow, Russia)
Schriver, D.
(NASA Headquarters Washington, DC United States)
Ashour-Abdalla, M.
(California Univ. Los Angeles, United States)
Date Acquired
August 16, 2013
Publication Date
January 1, 1993
Publication Information
Publication: Journal of Geophysical Research
Volume: 98
Issue: A1
ISSN: 0148-0227
Subject Category
Geophysics
Accession Number
93A23176
Funding Number(s)
CONTRACT_GRANT: NAGW-78
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available