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Relation of Microwave Emission to X-Ray Emission from Solar Flares

Published online by Cambridge University Press:  14 August 2015

Tatsuo Takakura
Tatsuo Takakura*
Affiliation:
Dept. of Astronomy, University of Tokyo, Japan

Abstract

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Recent observations of impulsive microwave and hard X-ray emissions during the early phase of the flares are briefly reviewed in order to deduce the dynamics of energetic electrons consistently from two view points of the microwaves and X-rays. An emphasis is put on the necessity of distinction between temporal and spatial variations so far confused in the interpretation of the time histories of the X-ray and radio emissions. The role of plasma turbulence on the dynamics of the energetic electrons is shown to be important in deducing the model of X-ray and radio sources.

Type
Part 3: Solar Flares
Information
Symposium - International Astronomical Union , Volume 68: Solar X, Gamma, and EUV Radiation , 1975 , pp. 299 - 313
Copyright
Copyright © Reidel 1975 

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