No CrossRef data available.
Article contents
Migration of polar prominences in 13-24 cycles of activity
Published online by Cambridge University Press: 27 November 2018
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.
We are performed the digitization of the prominences from the full disk observations of the Sun in the CaIIK line Kodaikanal Observatory for the period 1904-1954. These data were supplemented by digitization of prominences data on Wolfer atlases for the period 1887-1900 and observations of Kislovodsk Observatory in the period 1957-2017. Particular attention was paid to study of the polar crown prominences drift time. The time interval of the prominence drift is ambiguous from the sunspot cycle amplitude.
- Type
- Contributed Papers
- Information
- Copyright
- Copyright © International Astronomical Union 2018
References
Wolfer, A. Publikationen der Sternwarte des eidg. Polytechnikums zu Zurich.4 Bande Schulthess, Zurich, 1897;1899;1902;1909.Google Scholar
You have
Access