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Solar Radio S-Component Variation with the Magnetic Field of Active Regions

Published online by Cambridge University Press:  12 April 2016

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

Abstract

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According to an active region model proposed in the present paper, i.e. three-dimensional and continuous distributions of the three plasma parameters (electron temperature, electron density, and magnetic field) from the active region to the quiet region, and using the combined mechanisms of gyroresonance radiation and bremsstrahlung, we have researched the solar radio S-component (i.e. the slowly varying component or SVC) variation with the magnetic field of active regions.

Type
Session 5. Fields in the Chromosphere and Corona
Information
International Astronomical Union Colloquium , Volume 141: The Magnetic and Velocity Fields of Solar Active Regions , 1993 , pp. 275 - 278
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Zhao, R.-y. 1991a, Science in China ( Series A ), 34, 969 Google Scholar
Zhao, R.-y. 1991b, Science in China ( Series A ), 34, 1109 Google Scholar
Zhao, R.-y. 1991c, in The 1st China-Japan Seminar on Solar PhysicsGoogle Scholar