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Long-Term Coherent Periodicities in the Mean Magnetic Field of the Sun

Published online by Cambridge University Press:  04 August 2017

V.A. Kotov  and
L.S. Levitsky
V.A. Kotov
Affiliation:
Crimean Astrophysical Observatory Nauchny, Crimea 334413, USSR
L.S. Levitsky
Affiliation:
Crimean Astrophysical Observatory Nauchny, Crimea 334413, USSR

Extract

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To investigate periodic variations of the magnetic field of the Sun as a star (SMMF; see Severny, 1969) we have used the mean field measurements made in Crimea, Mt. Wilson, and Stanford observatories; in total N = 5783 daily values were available for the time interval 1968–1981. In essence, these data offer a unique possibility to study the Sun as a variable magnetic star (Scherrer et al., 1977).

Type
I. Magnetic Fields in Stellar Photospheres
Information
Symposium - International Astronomical Union , Volume 102: Solar and Stellar Magnetic Fields: Origins and Coronal Effects , 1983 , pp. 23 - 27
Copyright
Copyright © Reidel 1983 

References

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