Electron cyclotron maser emission at oblique angles

Details Electron cyclotron maser emission at oblique angles Electron cyclotron maser emission at oblique angles

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993p%26ss...41..333m&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 41, no. 5, p. 333-339.

Physics

7

Cyclotron Resonance, Electron Cyclotron Heating, Jupiter (Planet), Maser Outputs, Planetary Radiation, Radio Emission, Decametric Waves, Electron Acceleration, Elliptical Polarization, Jupiter, Emissions, Decimeter Waves, Radio Bursts, Polarization, Model, Velocity, Resonance, Calculations, Electrons, Distribution, Absorption, Energy, Acceleration, Trapping, Position (Location)

Scientific paper

Possible causes of observations of electron cyclotron maser emissions (ECMEs) at oblique angle (about 60 deg) to the magnetic field are investigated. The paper discusses general concepts of ECME in terms of resonant ellipses and considers electron distributions required to produce ECME at oblique angles, as well as the ways in which the most favorable of these distributions may be produced. A mechanism is proposed that might produce an appropriate 'spiraling beam' distribution, with a peak in velocity space at speed v - v(0) and pitch angle alpha = alpha(0) not equal to 0.

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