Method of Estimating Langmuir's Turbulence in a Solar Flare
Abstract
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.
- Publication:
-
Bulletin of the Astronomical Institutes of Czechoslovakia
- Pub Date:
- March 1983
- Bibcode:
- 1983BAICz..34..100K
- Keywords:
-
- Distribution Functions;
- Electrostatic Waves;
- Plasma Turbulence;
- Solar Flares;
- Solar Radio Bursts;
- Electron Energy;
- Microwaves;
- Plasma Physics;
- Solar Physics;
- Solar X-Rays;
- Solar Physics