Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-27T23:48:30.940Z Has data issue: false hasContentIssue false
  • English
  • Français

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

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.

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