Hydrodynamic model for generation of global poloidal flow of the Sun

1Loginov, AA, 1Salnikov, NN, 1Cheremnykh, OK, 2Krivodubskij, VN, 1Maslova, NV
1Space Research Institute of the National Academy of Sciences of Ukraine and the State Space Agency of Ukraine, Kyiv, Ukraine
2Astronomical Observatory of the Taras Shevchenko National University of Kyiv, Kyiv, Ukraine
Kosm. nauka tehnol. 2011, 17 ;(1):29-35
Publication Language: Russian
We propose the semi-empirical hydrodynamic model for global poloidal flow generation caused by the instability of the solar differential rotation. Spatial modes and increment of poloidal flow are determined.
Keywords: differential rotation, hydrodynamic model, poloidal flow
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