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Solar dynamo model with nonlocal alpha-effect and diamagnetic pumping

Published online by Cambridge University Press:  18 July 2013

L. L. Kitchatinov
Affiliation:
Institute for Solar-Terrestrial Physics, Lermontov Str. 126a, PO Box 291, Irkutsk 664033, Russia email: kit@iszf.irk.ru; osv@iszf.irk.ru Pulkovo Astronomical Observatory, St. Petersburg 196140, Russia
S. V. Olemskoy
Affiliation:
Institute for Solar-Terrestrial Physics, Lermontov Str. 126a, PO Box 291, Irkutsk 664033, Russia email: kit@iszf.irk.ru; osv@iszf.irk.ru
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Abstract

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Sunspot data and large-scale solar magnetic field data are used to demonstrate the operation of the Babcock-Leighton mechanism on the Sun. A dynamo model is developed that employs jointly a nonlocal alpha-effect of the Babcock-Leighton type and diamagnetic downward pumping. The pumping concentrates magnetic fields to the base of the convection zone. The magnetic cycle period, equatorial symmetry of the generated fields, their meridional drift, and the polar-to-toroidal field ratio obtained in the model agree with observations.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2013 

References

Dasi-Espuig, M., Solanki, S. K., Krivova, N. A., Cameron, R., & Peñuela, T. 2010, A&A, 518, A7 Google Scholar
Chatterjee, P., Nandy, D., & Choudhuri, A. R. 2004, A&A, 427, 1019 Google Scholar
Kitchatinov, L. L. & Olemskoy, S. V. 2011, MNRAS, 411, 1059 Google Scholar
Makarov, V. I., Tlatov, A. G., Callebaut, D. K., Obridko, V. N., & Shelting, B. D. 2001, Solar Phys., 198, 409 CrossRefGoogle Scholar