Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Electron cyclotron wave generation by relativistic electrons

Journal Article · · Journal of Geophysical Research; (United States)
DOI:https://doi.org/10.1029/93JA02319· OSTI ID:6720665
 [1];  [2]
  1. Southwest Research Institute, San Antonio, TX (United States)
  2. NASA/Goddard Space Flight Center, Greenbelt, MD (United States)
The authors show that an energetic electron distribution which has a temperature anisotropy (T[sub [perpendicular]b] > T[sub [parallel]b]), or which is gyrating about a DC magnetic field, can generate electron cyclotron waves with frequencies below the electron cyclotron frequency. Relativistic effects are included in solving the dispersion equation and are shown to be quantitatively important. The basic idea of the mechanism is the coupling of the beam mode to slow waves. The unstable electron cyclotron waves are predominantly electromagnetic and right-hand polarized. For a low-density plasma in which the electron plasma frequency is less than the electron cyclotron frequency, the excited waves can have frequencies above or below the electron plasma frequency, depending upon the parameters of the energetic electron distribution. This instability may account for observed Z mode waves in the polar magnetosphere of the Earth and other planets. 26 refs., 6 figs.
OSTI ID:
6720665
Journal Information:
Journal of Geophysical Research; (United States), Journal Name: Journal of Geophysical Research; (United States) Vol. 99:A1; ISSN JGREA2; ISSN 0148-0227
Country of Publication:
United States
Language:
English