Thermal Convection, Magnetic Field, and Differential Rotation in Solar-Type Stars PDF ePub eBook

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Thermal Convection, Magnetic Field, and Differential Rotation in Solar-Type Stars free pdf 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 layer. The author attacked this problem with a newly developed approach, the reduced speed of sound technique, which enabled him to investigate the surface and deep solar layers in a self-consistent manner. This technique also made it possible to achieve an unprecedented performance in the solar convection simulations for the usage of the massively parallel supercomputers such as the RIKEN K system. It was found that the turbulence and the mean flows such as the differential rotation and the meridional circulation mutually interact with each other to maintain the flow structures in the Sun. Recent observations by helioseismology support the author's proposed theoretical mechanism. The book also addresses the generation of the magnetic field in such turbulent convective motions, which is an important step forward for solar cyclic dynamo research.

About Hideyuki Hotta

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Details Book

Author : Hideyuki Hotta
Publisher : Springer Verlag, Japan
Data Published : 26 January 2015
ISBN : 4431553983
EAN : 9784431553984
Format Book : PDF, Epub, DOCx, TXT
Number of Pages : 81 pages
Age + : 15 years
Language : English
Rating :

Reviews Thermal Convection, Magnetic Field, and Differential Rotation in Solar-Type Stars



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