On spatial variations of magnetic field and superthermal electron distribution in cm-radio burst source

Details On spatial variations of magnetic field and superthermal electron distribution in cm-radio burst source On spatial variations of magnetic field and superthermal electron distribution in cm-radio burst source

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009iaus..257..353y&link_type=abstract

Universal Heliophysical Processes, Proceedings of the International Astronomical Union, IAU Symposium, Volume 257, p. 353-356

Astronomy and Astrophysics

Astronomy

Sun: Radio Radiation Methods: Data Analysis

Scientific paper

The paper presents a new method of an estimation of spatial variations of the magnetic field and superthermal electron distribution in solar cm-radio burst sources. The method is based on the analysis of several burst spectra recorded in the different moments of time and on the minimization of the difference between the theoretical and observed radio fluxes. It is found that the measure of the spatial variations of superthermal electron distribution in the radio source is always greater than that for the magnetic field. In most cases this measure has a minimum at the impulsive phase of cm-radio bursts.

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