NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Observational dispersion relationsPulse propagation in plasmas has been widely studied in relation to instabilities and their classification as convective or absolute. Such analyses emphasize the importance of considering the summation of a spectrum of modes, rather than simply making deductions from Brillouin dispersion relations plotted either for real frequency and complex wavenumber, or for complex frequency and real wavenumber. In particular, erroneous conclusions may be drawn about the magnitude and direction of propagation of a transient pulse. In this paper, the point of view is taken that an observer remote from the source would measure an 'observational dispersion relation'. The nature of this dispersion relation is examined for absorbing or convectively unstable plasmas by asymptotic analysis, and for different source waveforms. Illustrative results are presented for propagation in cold plasmas and for beam-plasma interaction.
Document ID
19820054061
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Crawford, F. W.
(Stanford Univ. CA, United States)
Vidmar, R. J.
(Stanford University Stanford, CA, United States)
Date Acquired
August 10, 2013
Publication Date
June 1, 1982
Subject Category
Plasma Physics
Accession Number
82A37596
Distribution Limits
Public
Copyright
Other

Available Downloads

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