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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
Extract
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
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- Copyright © Reidel 1983
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