Method of estimating Langmuir's turbulence in a solar flare

Details Method of estimating Langmuir's turbulence in a solar flare Method of estimating Langmuir's turbulence in a solar flare

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983baicz..34..100k&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 34, March 1983, p. 100-102.

Physics

Plasma Physics

Distribution Functions, Electrostatic Waves, Plasma Turbulence, Solar Flares, Solar Radio Bursts, Electron Energy, Microwaves, Plasma Physics, Solar Physics, Solar X-Rays

Scientific paper

In principle, the theory of X hard and microwave solar bursts makes it possible to determine the development of the 'mean' distribution function of hot or superthermal electrons during the impulse phase of a flare. On the basis of this development of the distribution function of electrons, the method described in this paper can be used to determine the parameters of Langmuir's turbulence, assumed to exist in a solar flare.

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