Negative magnetic buoyancy and formation of a sunspot belt
Magnetic buoyancy constrains the magnitude of toroidal field excited by the Ω-effect near the bottom of the solar convection zone (SCZ). Therefore, we examined two negative magnetic buoyancy effects: i) macroscopic turbulent diamagnetism (the γ-effect) and ii) magnetic advection caused by vertical i...
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| Date: | 2005 |
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| Main Author: | |
| Format: | Article |
| Language: | English |
| Published: |
Головна астрономічна обсерваторія НАН України
2005
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| Series: | Кинематика и физика небесных тел |
| Subjects: | |
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| Journal Title: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Cite this: | Negative magnetic buoyancy and formation of a sunspot belt / V.N. Kryvodubskyj // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 155-158. — Бібліогр.: 18 назв. — англ. |
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