Solar Poloidal Magnetic Field Generation Rate from Observations and Mean-Field Dynamos
Author:
Funder
the Ministry of Science and Higher Education of the Russian Federation
Publisher
Springer Science and Business Media LLC
Link
https://link.springer.com/content/pdf/10.1007/s11207-024-02357-0.pdf
Reference26 articles.
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2. Brandenburg, A.: 2005, The case for a distributed solar dynamo shaped by near-surface shear. Astrophys. J. 625, 539.
3. Brandenburg, A., Elstner, D., Masada, Y., Pipin, V.V.: 2023, Turbulent processes and mean-field dynamo. Space Sci. Rev. 219, 55. DOI. ADS.
4. Cameron, R.H., Schüssler, M.: 2023, Observationally guided models for the solar dynamo and the role of the surface field. Space Sci. Rev. 219, 60. DOI. ADS.
5. Charbonneau, P., Sokoloff, D.D.: 2023, Evolution of solar and stellar dynamo theory. Space Sci. Rev. 219, 35. DOI. ADS.
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