期刊
ASTROPHYSICAL JOURNAL
卷 544, 期 1, 页码 L79-L82出版社
UNIV CHICAGO PRESS
DOI: 10.1086/317291
关键词
hydrodynamics; MHD; Sun : interior; Sun : magnetic fields; Sun : rotation
We argue that the classical shallow water equations of geo]physical fluid dynamics should be useful for studying the global dynamics of the solar tachocline and demonstrate the existence of an MHD analog that would allow taking into account the strong toroidal magnetic field likely to be present there.
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