Thermal Convection, Magnetic Field, and Differential Rotation in Solar-type Stars
This thesis describes the studies on the solar interior where turbulent thermal convection plays an important role. The author solved, for the first time, one of the long-standing issues in solar physics, i.e., the maintenance mechanism of the solar differential rotation in the near-surface shear la...
| Published in: | Springer eBooks |
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| Format: | eBook |
| Language: | English |
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Tokyo :
Springer Japan : Imprint: Springer,
2015.
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| Series: | Springer Theses, Recognizing Outstanding Ph.D. Research,
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| Subjects: | |
| Online Access: | http://dx.doi.org/10.1007/978-4-431-55399-1 Перейти в каталог НБ ТГУ |
Table of Contents:
- General Introduction
- Basic Equations and Development of Numerical Code
- Structure of Convection and Magnetic Field without Rotation
- Reproduction of Near Surface Shear Layer with Rotation
- Concluding Remarks
- Appendix.