Published 1991 | Version v1
Report Restricted

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).

Optional Information

Contract/Grant/Project number
Contract W-7405-ENG-48
Funding organization
USDOE, Washington, DC (USA).
Secondary number(s)
CONF-9104109--2.