Nonthermal planetary radio emissions: Theories and observations

Details Nonthermal planetary radio emissions: Theories and observations Nonthermal planetary radio emissions: Theories and observations

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ppcn.conf..101c&link_type=abstract

In ESA, Fourth International Toki Conference on Plasma Physics and Controlled Nuclear Fusion p 101-104 (SEE N94-22624 05-75)

Physics

Plasma Physics

7

Nonthermal Radiation, Planetary Ionospheres, Planetary Magnetospheres, Radio Emission, Magnetohydrodynamic Stability, Planetary Magnetic Fields, Plasma Jets, Radio Auroras

Scientific paper

Intense radio waves are emitted by several planets. A variety of Nonthermal Planetary Radio emissions (NPR) are observed. Recent theoretical research of NPR are reviewed covering: acceleration of particles by nonlinear potential structures, saturation of stimulated scattering by wave breaking or frequency shift of beam modes, and generation of plasma radiation by Langmuir turbulence. Theories and observations of nonthermal planetary radio emissions are summarized. A variety of NPR was observed by space and ground radio telescopes and the observed characteristics of five types of NPR are presented. The theories of generation mechanisms of NPR are discussed and recent theoretical research of NPR is summarized.

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