Fundamental wave of type III solar radio bursts and whistler waves

Details Fundamental wave of type III solar radio bursts and whistler waves Fundamental wave of type III solar radio bursts and whistler waves

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...75..277t&link_type=abstract

Solar Physics, vol. 75, Jan. 1982, p. 277-292.

Physics

6

Computerized Simulation, Electron Beams, Plasma Waves, Plasma-Particle Interactions, Solar Electrons, Type 3 Bursts, Whistlers, Anisotropy, Electron Distribution, Nonuniform Magnetic Fields, Solar Flux Density, Solar Magnetic Field, Velocity Distribution, Wave Excitation

Scientific paper

It is shown through a numerical simulation that both the whistler waves and plasma waves are excited by a common solar electron beam. The excitation of the whistler waves is attributed to the loss-cone distribution which arises at a later phase of the passage of the beam at a given height owing to a velocity dispersion in the electron beam with a finite length. It is thought highly probable that the fundamental of type III bursts is caused by the coalescence of the whistler waves and the plasma waves excited by a common electron beam. This is considered likely even though the plasma waves must suffer induced scatterings by thermal ions (in order to have small wave numbers) before the coalescence can occur.

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