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Waves and Oscillations in Magnetic Fluxtubes

Published online by Cambridge University Press:  08 February 2017

M.P. Ryutova
M.P. Ryutova*
Affiliation:
Institute of Nuclear Physics 630090 Novosibirsk, 90 USSR

Abstract

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According to observational data solar magnetic fields have a pronounced filamentary structure. Theoretical investigations of plasmas containing structured magnetic fields, including the study of the properties of these structures and their interactions with associated gas flows, are of great importance for our understanding of the basic processes in the solar atmosphere, whose structure and dynamics are dominated by magnetic fields. In the present review theoretical models of thin magnetic fluxtubes and their behaviour in the ambient plasma are discussed.

Type
IV. Magnetohydrodynamics of the Photosphere
Information
Symposium - International Astronomical Union , Volume 138: Solar Photosphere: Structure, Convection and Magnetic Fields , 1990 , pp. 229 - 249
Copyright
Copyright © Kluwer 1990 

References

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