Hostname: page-component-5cf477f64f-bmd9x Total loading time: 0 Render date: 2025-04-02T07:32:04.112Z Has data issue: false hasContentIssue false
  • English
  • Français

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

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.

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