Theoretical Models of Stellar Activity Cycles
نویسندگان
چکیده
منابع مشابه
Theoretical Basis of Stellar Activity Cycles
Numerical simulations of hydromagnetic turbulence in the presence of shear and/or convection have given us new clues as to how the solar dynamo might work. Simulations suggest that here is signiicant large-scale magnetic eld generation at the bottom of the convection zone, where the radial shear is largest. The nature of the dynamo in the simulations seems to be qualitatively similar to an-dyna...
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ژورنال
عنوان ژورنال: Proceedings of the International Astronomical Union
سال: 2012
ISSN: 1743-9213,1743-9221
DOI: 10.1017/s1743921314004785