Published June 1983
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Wave generation in the aurora
Description
Wave generation mechanisms by a number of free energy sources in the magnetosphere are discussed. These include the temperature difference between the plasma sheet and the tail lobes, the temperature anisotropy, and field aligned currents. It is shown that a number of wave-modes can be generated via a Weibel-type instability by the above free energy sources, also the production of Langmuir waves can be created by ion-acoustic turbulence. Various wave-particle interaction mechanisms are presented as possible processes for the production of high energy electrons which are responsible for the aurora. (author)
Availability note (English)
MF available from INIS under the Report Number.
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Additional details
Publishing Information
- Imprint Pagination
- 5 p.
- Report number
- RL--83-029
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 15001553
- Subject category
- S58: GEOSCIENCES;
- Descriptors DEI
- ANGULAR DISTRIBUTION; AURORAE; EARTH MAGNETOSPHERE; ELECTRIC CURRENTS; ELECTRONS; ENERGY SOURCES; GEOMAGNETIC FIELD; ION ACOUSTIC WAVES; MAGNETOTAIL; PLASMA SHEET; TEMPERATURE DEPENDENCE; TURBULENCE; WAVE PROPAGATION
- Descriptors DEC
- CURRENTS; DISTRIBUTION; EARTH ATMOSPHERE; ELEMENTARY PARTICLES; FERMIONS; ION WAVES; LEPTONS; MAGNETIC FIELDS; PLASMA WAVES