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Titlebook: Basic Mechanisms of Solar Activity; V. Bumba,J. Kleczek Book 1976 International Astronomical Union 1976 Corona.Main sequence.Photosphere.R

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https://doi.org/10.1007/978-3-319-20212-9We investigated the reality of the differences in rotation rates found from various features. We only used published observations including almost forgotten work of more than half a century ago.
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Herman Heijermans and His DramasThe rotation law of the Sun is often described by the Faye formula:.where . is a heliographic latitude and . and . are constants. For a long time researchers have been studying the problem in what way the constants . and . change in time and in dependence on a phase of 11-year cycles.
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Hermann Abert — eine LebensbeschreibungI am going to show two slides which should clearly prove that sunspots are drifting very regularly in the north-south direction on the solar surface.
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Fast Variations of the Solar RotationThe rotation law of the Sun is often described by the Faye formula:.where . is a heliographic latitude and . and . are constants. For a long time researchers have been studying the problem in what way the constants . and . change in time and in dependence on a phase of 11-year cycles.
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Some Results of the Space Distribution of the Activation Vector of the Filaments in the 11-Year CyclIn 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.
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