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...
Κύριος συγγραφέας: | |
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Συγγραφή απο Οργανισμό/Αρχή: | |
Μορφή: | Ηλεκτρονική πηγή Ηλ. βιβλίο |
Γλώσσα: | English |
Έκδοση: |
Tokyo :
Springer Japan : Imprint: Springer,
2015.
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Σειρά: | Springer Theses, Recognizing Outstanding Ph.D. Research,
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Θέματα: | |
Διαθέσιμο Online: | Full Text via HEAL-Link |
Πίνακας περιεχομένων:
- 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.