The filamentary structure of the sunspot magnetic fields

Details The filamentary structure of the sunspot magnetic fields The filamentary structure of the sunspot magnetic fields

Jun 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974prama...2..327p&link_type=abstract

Pramana, vol. 2, June 1974, p. 327-335.

Physics

Condensed Matter

Statistical Mechanics

1

Electron Bunching, Fine Structure, Solar Magnetic Field, Solar Radio Bursts, Statistical Mechanics, Sunspots, Coherent Radiation, Electron Gas, Irreversible Processes, Magnetic Storms, Nonequilibrium Plasmas, Self Consistent Fields, Solar Activity, Solar Radiation, Type 3 Bursts

Scientific paper

The filamentary structure of the magnetic fields as well as the coherent radiations that emanate from a sunspot are explained, considering the solar burst as a nonequilibrium process. Methods of irreversible statistical mechanics have been applied to the problem of an electron gas in a constant magnetic field to explain the above features. We have obtained the nonequilibrium distribution function in the self-consistent field approximation. The dielectric function we obtained is a function of time, besides being a function of frequency and wave vector. We have thus taken the nonlinearity of the system as well. This theory explains many features of stria bursts, chain bursts, as well as the type III bursts.

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