Abstract
Eliminating the termN L, useful formulae for the magnetic field estimation in microwave radio sources are presented. Applications of these formulae to observed solar microwave radio bursts are shown.
This is a preview of subscription content, log in via an institution to check access.
References
Bastian, T.S. and Gary, D.E.: 1992,Solar Phys. 139, 357.
Batchelor, D.A., Benz, A.O. and Wiehl, H.J.: 1984,Astrophys. J. 280, 879.
Dulk, G.A.: 1985,Ann. Rev. Astron. Astrophys. 23, 169.
Dulk, G.A. and March, K.A.: 1982,Astrophys.J. 259, 350.
Gary, D.E.: 1985,Astrophys. J. 297, 799.
Lang, K.R.: 1980,Astrophysical Formulae, Springer-Verlag, New York.
Lim, J., White, S.M., Kundu, M.R. and Gary, D.E.: 1992,Solar Phys. 140, 343.
Tandberg-Hanssen, E. and Emslie, G.A.: 1988,The Physics of Solar Flares, Cambridge Univ. Press., Cambridge.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Ai-hua, Z., Karlický, M. Magnetic field estimation in microwave radio sources. Sol Phys 153, 441–444 (1994). https://doi.org/10.1007/BF00712516
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00712516