Abstract
We present expressions which describe the angular displacement of radio sources due to refraction in a magnetized plasma. The main objective of the present paper is to take into account the combined effect of gradients of the electron density and the magnetic field. We use the geometrical optics approximation for the determination of the angular broadening of the radiation. The expressions obtained axe applied to the case of the solar corona.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Baum, W.A. and Code, A.D.: 1953, Astron. Journ. 58, 108.
de Pater, I. and Ip, W.-H.: 1984,, Astrophys. Journ. 283, 895.
Ginsburg, B.L.: 1967, Electromagnetic Waves in Plasmas, Science, Moscow.
Parker, E.N.:1965, Interplanetary Dynamical Processes, Mir, Moscow.
Soboleva, N.S. and Timofeeva, G.M.: 1983, Soviet Astron. Lett. 9, 409.
Stelzried, C.T., Levy, G.S., Sato, T., Rusch, W.V.T., Ohlson, J.E., Schatten, K.H., and Wilcox, J.M.:1970, Solar Physics 14, 440.
Wright, C.S. and Nelson, G.J.: 1979, Icarus 38, 123.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1996 Kluwer Academic Publishers
About this paper
Cite this paper
Gnedin, Y.N., Lopez, E.D. (1996). Magnetic Polarimetric Refraction in the Solar Corona. In: Stenflo, J.O., Nagendra, K.N. (eds) Solar Polarization. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0231-2_8
Download citation
DOI: https://doi.org/10.1007/978-94-009-0231-2_8
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-6586-3
Online ISBN: 978-94-009-0231-2
eBook Packages: Springer Book Archive