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On the Origin of Microwave Emission from Sunspots

Published online by Cambridge University Press:  14 August 2015

R. Pallavicini
R. Pallavicini*
Affiliation:
Arcetri Astrophysical Observatory, Florence, Italy

Abstract

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Coordinated high-resolution XUV and centimetric observations of active regions obtained from Skylab and Stanford are compared with the aim of determining the nature of the centimetric radiation. It is concluded that the thermal gyroresonance process is the most likely emission mechanism for the bright compact radio sources associated with sunspots.

Type
Session II - Active Regions
Information
Symposium - International Astronomical Union , Volume 86: Radio Physics of the Sun , 1980 , pp. 119 - 122
Copyright
Copyright © Reidel 1980 

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