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On the Origin of Microwave Emission from Sunspots
Published online by Cambridge University Press: 14 August 2015
Abstract
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