Solar Cycle Structure and Structure of Activity Cycles at Late-Type Stars

It is shown that a description of the solar cycle using the odd zonal harmonic of the solar magnetic field expands our capabilities in two important areas of solar research: first, in improving and expanding the forecast to the near future of evolution of the cyclic solar activity and, second, in de...

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Veröffentlicht in:	Astronomy reports 2023-12, Vol.67 (12), p.1442-1451
Hauptverfasser:	Obridko, V. N., Sokoloff, D. D., Katsova, M. M.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Magnetic fields Observations and Techniques Physics Physics and Astronomy Solar activity Solar cycle Solar magnetic field Spectrophotometry Stellar magnetic fields
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Beschreibung
Zusammenfassung:	It is shown that a description of the solar cycle using the odd zonal harmonic of the solar magnetic field expands our capabilities in two important areas of solar research: first, in improving and expanding the forecast to the near future of evolution of the cyclic solar activity and, second, in developing a program for monitoring the spectrophotometric characteristics of radiation of solar-like stars, aimed at obtaining new information about their magnetic fields.
ISSN:	1063-7729 1562-6881
DOI:	10.1134/S1063772923120065