NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Three-dimensional simulation of whistler mode excited by the Spacelab 2 electron beamDuring the Spacelab 2 mission, while an electron beam was being ejected from the Shuttle, the Plasma Diagnostics Package (PDP) detected a clear funnel-shaped emission that is believed to be caused by whistler-mode emission from the electron beam. In order to understand the mechanism of this emission, simulations with a three-dimensional partially magnetostatic code have been performed. The simulation results show that whistler-mode and lower hybrid waves are excited by the electron beam, which is initially localized in the column in the three-dimensional simulation system, and that they propagate away from the beam. The wave spectra of the electric and magnetic fields diagnosed at some points show several peaks due to the waves excited by the electron beam. The frequency range of these spectra is in qualitative agreement with the PDP data. The intense narrowband electrostatic emission near the electron plasma frequency is observed by the simulations. The simulation results show that the beam instability is responsible for the generation mechanism of these emissions.
Document ID
19890056308
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Nishikawa, K.-I.
(Iowa Univ. Iowa City, IA, United States)
Frank, L. A.
(Iowa Univ. Iowa City, IA, United States)
Huang, C. Y.
(Iowa, University Iowa City, United States)
Date Acquired
August 14, 2013
Publication Date
June 1, 1989
Publication Information
Publication: Journal of Geophysical Research
Volume: 94
ISSN: 0148-0227
Subject Category
Geophysics
Accession Number
89A43679
Funding Number(s)
CONTRACT_GRANT: NAGW-1239
CONTRACT_GRANT: N00014-88-K-2007
CONTRACT_GRANT: NSF ATM-85-19528
Distribution Limits
Public
Copyright
Other

Available Downloads

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