Solar turbulent dynamo near convective overshoot layer and radiative tachocline
In order to extend the abilities of the αΩ-dynamo model to explain the observed regularities and anomalies of the solar magnetic activity, the magnetic quenching of the α-effect were included in the model, and newest helioseismically determined inner rotation of the Sun has been used. Allowance for...
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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/123456789/79616 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Zitieren: | Solar turbulent dynamo near convective overshoot layer and radiative tachocline / V.N. Kryvodubskyj // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 117-123. — Бібліогр.: 51 назв. — англ. |