On meridional Circulation in Stars
نویسندگان
چکیده
منابع مشابه
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A quasi-steady-state model of the consequences of rotation on the hydrodynamical structure of a stellar radiative zone is derived by studying in particular the role of centrifugal and baroclinic driving of meridional motions in angular momentum transport. This non-linear problem is solved numerically, assuming axial symmetry of the system, and within some limits it is shown that there exist sim...
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ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 2000
ISSN: 0074-1809
DOI: 10.1017/s0074180900167154