A method of the coronal magnetic field strength estimation from the microwave burst spectrum at the optically thin part.

Details A method of the coronal magnetic field strength estimation from the microwave burst spectrum at the optically thin part. A method of the coronal magnetic field strength estimation from the microwave burst spectrum at the optically thin part.

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995acasn..36..216z&link_type=abstract

Acta Astron. Sin., Vol. 36, No. 2, p. 216 - 219

Astronomy and Astrophysics

Astronomy

Solar Microwave Bursts: Magnetic Fields, Solar Magnetic Fields: Methods Of Reduction

Scientific paper

An approximate formula of the magnetic field strength in microwave burst sources is presented based on some simplified expressions for the gyrosynchrotron radiation. On the approximate formula the magnetic field estimation only depends on the observations of the microwave burst spectrum at the optically thin part, additional assumptions or data are unnecessary. For a set of appropriate parameters of the microwave burst spectrum the magnetic field strength was estimated and its error was given.

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