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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Bibliographic Details
Published in:Astronomy reports 2023-12, Vol.67 (12), p.1442-1451
Main Authors: Obridko, V. N., Sokoloff, D. D., Katsova, M. M.
Format: Article
Language:English
Subjects:
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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Summary: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