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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
Abstract
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
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- Copyright © Astronomical Society of the Pacific 1993
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