Published 1991
| Version v1
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Quasilinear simulation of auroral kilometric radiation by a relativistic Fokker-Planck code
Description
An intense terrestrial radiation called the auroral kilometric radiation (AKR) is believed to be generated by cyclotron maser instability. We study a quasilinear evolution of this instability by means of a two-dimensional relativistic Fokker-Planck code which treats waves and distributions self-consistently, including radiation loss and electron source and sink. We compare the distributions and wave amplitude with spacecraft observations to elucidate physical processes involved. 3 refs., 1 fig
Availability note (English)
MF available from INIS under the Report Number; OSTI as DE91009736; NTIS; INIS; US Govt. Printing Office Dep.
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Additional details
Publishing Information
- Imprint Pagination
- 5 p.
- Report number
- UCRL-JC--106422
Conference
- Title
- 4. international school for space simulation.
- Dates
- 1-5 Apr 1991.
- Place
- Nara (Japan).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 22050463
- Subject category
- S58: GEOSCIENCES;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- AURORAE; CYCLOTRON INSTABILITY; CYCLOTRON RADIATION; ELECTRON SOURCES; FINITE ELEMENT METHOD; FOKKER-PLANCK EQUATION; PLASMA SIMULATION; PLASMA WAVES; RELATIVISTIC RANGE
- Descriptors DEC
- BREMSSTRAHLUNG; DIFFERENTIAL EQUATIONS; ELECTROMAGNETIC RADIATION; ENERGY RANGE; EQUATIONS; INSTABILITY; NUMERICAL SOLUTION; PARTIAL DIFFERENTIAL EQUATIONS; PARTICLE SOURCES; PLASMA INSTABILITY; PLASMA MICROINSTABILITIES; RADIATION SOURCES; RADIATIONS; SIMULATION
Optional Information
- Contract/Grant/Project number
- Contract W-7405-ENG-48
- Funding organization
- USDOE, Washington, DC (USA).
- Secondary number(s)
- CONF-9104109--2.