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The ‘detwisted’ prominence of September 12, 1966

Published online by Cambridge University Press:  14 August 2015

Boris Valniček
Boris Valniček*
Affiliation:
Astronomical Institute, Czechoslovak Academy of Sciences, Ondřejov, C.S.S.R.

Abstract

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The eruptive prominence of September 12, 1966, is described. Detwisting of two filaments is demonstrated and compared with similar phenomena and with tornado prominences. A short discussion of mechanisms of the origin and subsequent development of the phenomenon is given.

Type
Part III: Optical Structure of an Active Region
Information
Symposium - International Astronomical Union , Volume 35: Structure and Development of Solar Active Regions , 1968 , pp. 282 - 286
Copyright
Copyright © Reidel 1968 

References

Alfvén, H. (1955) in Cosmical Electrodynamics, p. 117.Google Scholar
Bostick, W. H. (1958) Rev. mod. Phys., 30, 1090.CrossRefGoogle Scholar
Carmichael, H. (1963) AAS-NASA Symposium on the Physics of Solar Flares, p. 451.Google Scholar
Gold, T. (1963) AAS-NASA Symposium on the Physics of Solar Flares, p. 389.Google Scholar
Petit, E. (1950) Publ. astr. Soc. Pacific, 62, 144.Google Scholar
Valníček, B., Godoli, G., Mazzucconi, F. (1968) IQSY-Annals, PFP-Project.Google Scholar