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On the Formulae for Calculating the Magnetic Field in the Source of Solar Microwave Bursts

Published online by Cambridge University Press:  12 April 2016

Ren-Yang Zhao*
Affiliation:
Beijing Observatory, Academia Sinica, Beijing 100080, China

Abstract

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Based on the theory of gyro-synchrotron radiation from both thermal and nonthermal electrons, and adopting the relation between the peak frequency and the corresponding rise time of microwave bursts, we have derived several analytical formulae for calculating the magnetic field in the source regions of solar microwave bursts.

Type
Session 5. Fields in the Chromosphere and Corona
Copyright
Copyright © Astronomical Society of the Pacific 1993

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