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Simulation study of the loss cone driven cyclotron maser applied to auroral kilometric radiation

Journal Article · · Radio Sci.; (United States)
The linear growth and nonlinear saturation of electromagnetic radiation amplified by a hot (5-20 keV) population of electrons possessing a loss cone velocity distribution in the presence of a cold (20-500 eV) electron population are studied. A relativistic electromagnetic simulation code is used to study the emission process. Three cases are presented in detail to illustrate the generation process of auroral kilometric radiation. The first case, which has an electron plasma frequency omega(pe) 0.2 omega(ce) (electron cyclotron frequency) and possesses a double loss cone distribution, exhibits a strong narrow peak of the fast extraordinary mode (X mode) radiation just above the X mode cutoff frequency. The second case with omega(pe) 0.2 omega(ce) and a single loss cone distribution shows a preferred direction of propagation for the amplified radiation. The third case with omega(pe) 0.5 omega(ce) shows a peak in the ordinary mode (O mode) radiation. In all cases, the radiation saturates by turbulent scattering of resonant particles into the loss cone. 22 references.
Research Organization:
Sandia National Lab., Albuquerque, NM
DOE Contract Number:
AT06-76ER70005; FG05-80ET53088
OSTI ID:
6447662
Journal Information:
Radio Sci.; (United States), Journal Name: Radio Sci.; (United States) Vol. 19; ISSN RASCA
Country of Publication:
United States
Language:
English