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Generation of Plasma Flows and Filamentation of Magnetic Fields in the Solar Atmosphere

Published online by Cambridge University Press:  12 April 2016

Margarita Ryutova
Margarita Ryutova*
Affiliation:
Institute of Nuclear Physics, 630090 Novosibirsk, 90, Russia

Abstract

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Nonlinear effects in dynamics of solar magnetic fields which, in particular, determine the evolution of solar magnetic structures and their lifetimes, are discussed. By some analogy with the effects of acoustic streaming in usual hydrodynamics the general definition of these effects as “magneto acoustic streaming” is proposed.

Type
Session 9. Convections and Oscillation in Active Regions
Information
International Astronomical Union Colloquium , Volume 141: The Magnetic and Velocity Fields of Solar Active Regions , 1993 , pp. 549 - 553
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Faraday, M., 1831, Phil. Trans. Roy. Soc. London, 121, 229.Google Scholar
Nyborg, W.L., 1965, in Physical Acoustics, Vol. 2, Part B, Properties of Polimers and Nonlinear Acoustics, Academic Press.Google Scholar
Rayleigh, Lord, 1884, Phil. Trans. Roy. Soc. London, 175, 1.Google Scholar
Ryutov, D.D., Ryutova M.P., , 1976, Sov. Phys. JETP, 43, 491.Google Scholar
Ryutova, M.P., 1977, XIII Int. Conf. on Phenomena in Ionized Gases, Berlin, p. 859.Google Scholar
Ryutova, M.P., 1986, Proc. of Joint Varenna-Abastumani Int. School on Plasma Astrophysics, ESA, p. 71.Google Scholar
Ryutova, M., Kaisig, M., Tajima, T., 1992, in preparation.Google Scholar