Hostname: page-component-78c5997874-8bhkd Total loading time: 0 Render date: 2024-11-17T23:36:10.747Z Has data issue: false hasContentIssue false
  • English
  • Français

Some Results of the Space Distribution of the Activation Vector of the Filaments in the 11-Year Cycle

Published online by Cambridge University Press:  14 August 2015

V. V. Kasinskij ,
G. Ya. Smolkov  and
G. N. Zubkova
V. V. Kasinskij
Affiliation:
Sibizmiran, Irkutsk, U.S.S.R.
G. Ya. Smolkov
Affiliation:
Sibizmiran, Irkutsk, U.S.S.R.
G. N. Zubkova
Affiliation:
Sibizmiran, Irkutsk, U.S.S.R.

Extract

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.

In order to obtain new information on the manifestation of basic mechanisms of solar activity with the sunspot cycle development we have studied peculiarities of the latitude-time distribution of activation positions and suddenly disappearing filaments with respect to sunspot groups of cycles 18 to 20.

Type
Part 1: Basic Observed Parameters of the Solar Cycle
Information
Symposium - International Astronomical Union , Volume 71: Basic Mechanisms of Solar Activity , 1976 , pp. 191 - 197
Copyright
Copyright © Reidel 1976 

References

1. Kasinskij, V. V.: 1973, Solar Data Bulletin , NN 2, 7, 1973.Google Scholar
2. Kasinskij, V. V. and Plusnina, L. A.: 1974, Issled. Geomag. Aeron. Fiz. Solnza 31, 44.Google Scholar
3. Cartes Synoptiques de la Chromosphère Solaire, Méudon, 1945–1973.Google Scholar
4. Quart. Bull. Solar Activity , Zürich, 1955–1973.Google Scholar