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Quantitative estimations of the anomalous plasma diffusion in an active region∗

Published online by Cambridge University Press:  14 August 2015

M. Kopecký  and
G. V. Kuklin
M. Kopecký
Affiliation:
Siberian Institute of Terrestrial Magnetism, Ionosphere and Radio Propagation, Academy of Sciences, Irkutsk, U.S.S.R.
G. V. Kuklin
Affiliation:
Siberian Institute of Terrestrial Magnetism, Ionosphere and Radio Propagation, Academy of Sciences, Irkutsk, U.S.S.R.

Abstract

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In some recent papers the interdependence of the gas and magnetic-field motions in the solar atmosphere was considered. Some results indicate the occurrence of gas motion along the magnetic-field lines combined with motion of the field line, but sometimes we have to assume an obvious gas motion across the magnetic-field lines. As one of the possible mechanisms explaining this fact the anomalous plasma diffusion may be proposed.

Type
Part II: Theoretical Aspects
Information
Symposium - International Astronomical Union , Volume 35: Structure and Development of Solar Active Regions , 1968 , pp. 131 - 133
Copyright
Copyright © Reidel 1968 

References

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