Some unresolved problems in the solar dynamo

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Published: Jun 15, 2022
Abstract views: 295
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DOI: https://doi.org/10.34898/aat.vol3.iss2.pp8-11
Keywords:
solar activity solar cycle stellar activity stellar cycles magnetic field generation

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D.D. Sokoloff
Moscow State University, Moscow 119991, Russia; IZMIRAN, Kaluzhskoe shosse 4, Troitsk 1421980, Russia; Moscow Center of Fundamental and Applied Mathematics, Moscow 119991, Russia

Abstract

Contemporary solar dynamo theory is now transiting to the solar activity prediction problems. It looks important however to keep in mind foundations of the solar dynamo theory. This is why we consider here some unresolved problems in these foundations. The problems are important for understanding solar activity as well as activity of stars similar to some extent to the Sun.

Supporting Agencies

The author is grateful to the Theoretical Physics and Mathematics Advancement Foundation “BASIS” (grant 21- 1-1-4-1) and the Ministry of Science and Higher Education (agreement 075-15-2019-1621) for financial support of the work.

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How to Cite
Sokoloff D. , 2022. Acta Astrophysica Taurica, vol. 3, no. 2, pp. 8–11. DOI: 10.34898/aat.vol3.iss2.pp8-11
Issue
Vol. 3 No. 2 (2022)
Section
Magnetism and activity of the Sun and stars – 2021 Conference proceedings

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References

Charbonneau P., St-Jean C., Zacharias P., 2005. Astrophys. J., vol. 619, no. 1, p. 613.

Choudhuri A.R., Karak B.B., 2012. Phys. Rev. Lett., vol. 109, no. 17, id. 171103.

Frick P. et al., 2020. Mon. Not. Roy. Astron. Soc., vol. 491, p. 5572.

Jennings R.L., Weiss N.O., 1991. Mon. Not. Roy. Astron. Soc., vol. 252, pp. 249–260.

Kalinin A., Sokoloff D., 2019. Magnetohydrodynamics, vol. 55, no. 1–2, p. 193.

Moss D. et al., 2002. Astron. Astrophys., vol. 396, p. 885. Sokoloff D. et al., 2020. Mon. Not. Roy. Astron. Soc., vol. 497, no. 4, p. 4376.

Stepanov R. et al., 2020. Mon. Not. Roy. Astron. Soc., vol. 495, no. 4, p. 3788.

Wu C.J. et al., 2018. Astron. Astrophys., vol. 615, id. A93.

Zhukova A. et al., 2020. Solar Phys., vol. 295, p. 165.