Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-27T07:44:45.113Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
Information
International Astronomical Union Colloquium , Volume 141: The Magnetic and Velocity Fields of Solar Active Regions , 1993 , pp. 295 - 298
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Batchelor, D.A., Crannell, C.J., Wiehl, H.J., & Magun, A. 1985, ApJ, 295, 258 Google Scholar
Brown, J.C., Melrose, D.B., & Spicer, D.S. 1979, ApJ, 228, 592 Google Scholar
Crannell, C.J., Frost, K.J., Matzler, C., Ohki, K., & Saba, J.L. 1978, ApJ, 223, 620 CrossRefGoogle Scholar
Dulk, G.A. 1985, ARA&A, 23, 169 Google Scholar
Dulk, G.A., Melrose, D.B., & White, S.M. 1979, ApJ, 234, 1137 Google Scholar
Smith, D.F. & Lilliequist, C.G. 1979, ApJ, 232, 582 Google Scholar
Zhao, R.-y., Magun, A., & Schanda, E. 1990, Solar Phys., 130, 361 CrossRefGoogle Scholar