Simulation studies of plasma waves in the electron foreshock: The generation of downshifted oscillations
Creators
- 1. Max Planck Inst. fuer Extraterrestrische Physik, Garching (West Germany)
- 2. Massachusetts Inst. of Tech., Cambridge (USA)
Description
The generation of waves with frequencies downshifted from the plasma frequency, as observed in the electron foreshock, is analyzed by particle simulation. Wave excitation differs fundamentally from the familiar excitation of the plasma eigenmodes by a gentle bump-on-tail electron distribution. Beam modes are destabilized by resonant interaction with bulk electrons, provided the beamvelocity spread is very small. These modes are stabilized, starting with the higher frequencies, as the beam is broadened and slowed down by the interaction with the wave spectrum. Initially, a very cold beam is also capable of exciting frequencies considerably above the plasma frequency, but such oscillations are quickly stabilized. Low-frequency modes persist for a long time, until the bump in the electron distribution is completely ironed out. This diffusion process also is quite different from the familiar case of well-separated beam and bulk electrons. A quantitative analysis of these processes is carried out
Additional details
Publishing Information
- Journal Title
- Journal of Geophysical Research
- Journal Volume
- 95
- Journal Issue
- A6
- Series
- J. Geophys. Res.
- Journal Page Range
- 8123-8131
- ISSN
- 0148-0227
- CODEN
- JGREA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 22089209
- Subject category
- S58: GEOSCIENCES;
- Descriptors DEI
- BEAM-PLASMA SYSTEMS; COMPUTERIZED SIMULATION; DIFFUSION; DISTRIBUTION FUNCTIONS; EARTH MAGNETOSPHERE; ELECTRON BEAMS; ELECTRONS; INTERACTIONS; INTERPLANETARY SPACE; LANGMUIR FREQUENCY; NUMERICAL SOLUTION; PLASMA WAVES; REFLECTION; SHOCK WAVES; SOLAR WIND; STABILITY
- Descriptors DEC
- BEAMS; EARTH ATMOSPHERE; ELEMENTARY PARTICLES; FERMIONS; LEPTON BEAMS; LEPTONS; PARTICLE BEAMS; SIMULATION; SOLAR ACTIVITY; SPACE; STELLAR ACTIVITY; STELLAR WINDS