On the possibility of supergiant stable flows in the convection zone of the sun

Tikhomolov, Evgeniy

doi:10.1007/3-540-58041-7_205

On the possibility of supergiant stable flows in the convection zone of the sun

Evgeniy Tikhomolov¹

Part II Generation of Large-Scale Magnetic Fields
Conference paper
First Online: 01 January 2005

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1 Citations

Part of the book series: Lecture Notes in Physics ((LNP,volume 432))

Abstract

We present a numerical model of convection in a rotating fluid layer with a deformable upper free surface, which exhibits a solution in the form of a large-scale dissipative structure.

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Authors and Affiliations

Institute of Solar Terrestrial Physics, P.O.Box 4026, 664033, Irkutsk, Russia
Evgeniy Tikhomolov

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Evgeniy Tikhomolov
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G. Belvedere M. Rodonò G. M. Simnett

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Tikhomolov, E. (1994). On the possibility of supergiant stable flows in the convection zone of the sun. In: Belvedere, G., Rodonò, M., Simnett, G.M. (eds) Advances in Solar Physics. Lecture Notes in Physics, vol 432. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-58041-7_205

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DOI: https://doi.org/10.1007/3-540-58041-7_205
Published: 20 July 2005
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-58041-6
Online ISBN: 978-3-540-48420-2
eBook Packages: Springer Book Archive

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