Waves and Oscillations in Magnetic Fluxtubes [chapter]

M. P. Ryutova
1990 Solar Photosphere: Structure, Convection, and Magnetic Fields  
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
more » ... thin magnetic fluxtubes and their behaviour in the ambient plasma are discussed. 229 J. O. Stenflo (ed.), Solar Photosphere: Structure, Convection, and Magnetic Fields, 229-249. © 1990 by the IAU. available at https://www.cambridge.org/core/terms. https://doi.
doi:10.1007/978-94-009-1061-4_24 fatcat:gc4k4a2z7zbfdczjss33tul32y