Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-29T17:29:16.027Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Galeev, A. A., Moiseev, S.S., Sagdeev, R.Z. (1963) Preprint, Novosibirsk.Google Scholar
Kopecký, M., Kuklin, G. V. (1966) Bull. astr. Inst. Csl., 17, 45.Google Scholar
Kopecký, M., Kuklin, G. V. (1968) Solar Phys., 4, in press.Google Scholar
Kuklin, G.V. (1966) Resultaty nabl. i issled. v period. MGSS, 1, 17.Google Scholar
Zwaan, C. (1965) Rech. astr. Obs. Utrecht, 17, 4.Google Scholar