NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Press Enter or click the Search button to begin your search.

Back to Results
Electron-cyclotron maser instability caused by hot electronsThe electron-cyclotron maser instability is studied for energetic electrons with a loss-cone distribution. The instability can occur at all angles of propagation for a wide range of parameters. The growth rate is significantly reduced by the presence of a population of cold electrons, and the instability can be suppressed if the density of the cold electrons is sufficiently large and the temperature of the energetic electrons is not too high.
Document ID
19850065468
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Wong, H. K.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Wu, C. S.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Gaffey, J. D., Jr.
(Maryland, University College Park, United States)
Date Acquired
August 12, 2013
Publication Date
September 1, 1985
Publication Information
Publication: Physics of Fluids
Volume: 28
ISSN: 0031-9171
Subject Category
Plasma Physics
Report/Patent Number
ISSN: 0031-9171
Accession Number
85A47619
Funding Number(s)
CONTRACT_GRANT: NGL-21-002-005
Distribution Limits
Public
Copyright
Other

Available Downloads

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