MHD spin-down of a G-type star-Reference-Cited by-同舟云学术

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MHD spin-down of a G-type star

Published:1996-12 Issue:3-4 Volume:83 Page:307-326
ISSN:0309-1929
Container-title:Geophysical & Astrophysical Fluid Dynamics
language:en
Short-container-title:Geophysical & Astrophysical Fluid Dynamics

Author:

Kitayama Osamu¹,Sakurai Takeo¹,Ma Jiefu¹

Affiliation:

1. a Division of Aeronautical and Astronautical Engineering, Faculty of Engineering , Kyoto University , Kyoto

Publisher

Informa UK Limited

Subject

Geochemistry and Petrology,Mechanics of Materials,Geophysics,Astronomy and Astrophysics,Computational Mechanics

Link

https://www.tandfonline.com/doi/pdf/10.1080/03091929608208970

Reference26 articles.

1. On the instability of toroidal magnetic fields and differential rotation in stars

2. Local analysis of thermal and magnetic instabilities in a rapidly rotating fluid

3. Solar rotation as a function of depth and latitude

4. Phase-mixing and surface waves: a new interpretation

Cited by 1 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. The slender solar tachocline: a magnetic model;ASTRON NACHR;1997

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