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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

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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