Evolution of large-scale magnetic fields in the Sun
A scenario of evolution of the large-scale magnetic fields in the Sun is proposed. The analysed models of the Sun allow one to accept the shearing of the poloidal field by differential rotation, helical turbulence and also the advective transport of the magnetic flux by meridional circulation as the...
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| Veröffentlicht in: | Кинематика и физика небесных тел |
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| Datum: | 2005 |
| 1. Verfasser: | |
| Format: | Artikel |
| Sprache: | English |
| Veröffentlicht: |
Головна астрономічна обсерваторія НАН України
2005
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| Schlagworte: | |
| Online Zugang: | https://nasplib.isofts.kiev.ua/handle/123456789/79637 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Zitieren: | Evolution of large-scale magnetic fields in the Sun / P.G. Brayko // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 176-178. — Бібліогр.: 13 назв. — англ. |