Electromagnetic loss-cone instability and type IV solar radio bursts

Details Electromagnetic loss-cone instability and type IV solar radio bursts Electromagnetic loss-cone instability and type IV solar radio bursts

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pazh....4..193s&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 4, Apr. 1978, p. 193-196.) Soviet Astronomy Letters, vol. 4, Mar.-Apr. 1978, p. 103-106

Astronomy and Astrophysics

Astronomy

10

Energetic Particles, Magnetically Trapped Particles, Magnetohydrodynamic Stability, Plasma Waves, Solar Corona, Type 4 Bursts, Bessel Functions, Electron Distribution, Energy Dissipation, Plasma-Electromagnetic Interaction, Relativistic Particles, Synchrotron Radiation

Scientific paper

The loss-cone instability of electromagnetic waves at electron cyclotron
harmonics in coronal magnetic traps, the sources of type IV bursts, is
examined. If the magnetic field is strong enough, the linear mechanism
through which radio emission is generated by electrons of approximately
50 keV energy may predominate over the nonlinear plasma mechanism.

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