Note on fine structure of the 11-year solar cycle.

Physics

Scientific paper

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Scientific paper

On the basis of Greenwich data on mean total sunspot areas for a Carrington solar rotation characteristics of fine structure of solar cycles 18 - 20 have been obtained separately for the N and S hemispheres and for the entire solar disc. An analysis of the N-S asymmetry at the extrema of the fine structure of the cycle for solar cycles 12 - 20 shows that the sunspot secular cycle essentially influences the fine structure of the sunspot 11-year cycle.

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