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The Possibility of Magnetic Field Origin in Fine Structure Elements of Solar Features

Published online by Cambridge University Press:  14 August 2015

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

Abstract

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It is demonstrated that in principle the magnetic field may originate in the fine structure elements of the photosphere and the sunspots as a result of lack of coincidence of isobaric and isothermic surfaces in those elements.

Type
Part V: Theories of Small Scale Magnetic Fields
Information
Symposium - International Astronomical Union , Volume 43: Solar Magnetic Fields , 1971 , pp. 534 - 541
Copyright
Copyright © Reidel 1971 

References

de Jager, C.: 1959, Handbuch der Astrophysik , Bd. 52, p. 83.Google Scholar
Kopecký, M. and Kuklin, G. V.: 1967, Bull. Astron. Inst. Czech. 18, 77.Google Scholar
Kopecký, M. and Kuklin, G. V.: 1969, Solar Phys. 6, 241.Google Scholar
Kuklin, G. V.: 1966, Rezultaty nabl. i issled. v period MGSS , vyp. I ‘Nauka’ Moskva, p. 17.Google Scholar
Obridko, V. N.: 1968, Bull. Astron. Inst. Czech. 19, 183.Google Scholar
Teplitzkaya, R. B.: 1970, Private Communication.Google Scholar
Wilson, P. R.: 1969, Solar Phys. 10, 404.CrossRefGoogle Scholar