Study of the Periodicities of the Solar Differential Rotation
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 reveal...
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| Veröffentlicht in: | Astrophysics 2020-06, Vol.63 (2), p.282-287 |
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| container_title | Astrophysics |
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| creator | Japaridze, D. Dumbadze, G. Ramishvili, G. Chargeishvili, B. |
| description | 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. |
| doi_str_mv | 10.1007/s10511-020-09633-4 |
| format | Article |
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| language | eng |
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| subjects | Astronomy Astrophysical observatories Astrophysics Astrophysics and Astroparticles Astrophysics and Cosmology Differential rotation Filaments Hydrogen Magnetic fields Observations and Techniques Periodic variations Periodicities Physics Physics and Astronomy Solar activity Solar activity cycles Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics |
| title | Study of the Periodicities of the Solar Differential Rotation |
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