Data on solar hydrogen filaments obtained at the Abastumani Astrophysical Observatory during solar activity cycles 19-22 are used to study the characteristic periods of the solar differential rotation. In addition to the known 11-year period of solar activity, a quasi-biennial periodicity was revealed for the rotation rates of hydrogen filaments and a quasi-five-year periodicity was also found for the number of hydrogen filaments.
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Translated from Astrofizika, Vol. 63, No. 2, pp. 319-324 (May 2020)
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Japaridze, D., Dumbadze, G., Ramishvili, G. et al. Study of the Periodicities of the Solar Differential Rotation. Astrophysics 63, 282–287 (2020). https://doi.org/10.1007/s10511-020-09633-4
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DOI: https://doi.org/10.1007/s10511-020-09633-4