Generalized scenario for the evolution of solar cycles of weak photospheric and strong magnetic fields

Heading: 
Astronomy and Astrophysics
1Zyelyk, Ya.I, 2Stepanian, NN, 2Andryeyeva, OA
1Space Research Institute of the National Academy of Sciences of Ukraine and the State Space Agency of Ukraine, Kyiv, Ukraine
2Scientific-Research Institute “Crimean Astrophysical Observatory” of the Ministry for Education and Science of Ukraine, Nauchny, AR Crimea, Ukraine
Kosm. nauka tehnol. 2012, 18 ;(1):68–73
https://doi.org/10.15407/knit2012.01.068
Publication Language: Russian
Abstract: 
Based on observational data, the evolution of large-scale solar magnetic fields is studied over three solar cycles and the generalized scenario of the change for solar cycles of weak photospheric and strong (in active regions) fields is determined. It is found that, along with significant differences in the evolution of weak and strong magnetic fields, there is a close relation between their behaviors in the selected strength intervals, when the growth rate of the total field flux is considered as a characteristic for the comparison
Keywords: cycles, magnetic fields, Sun
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