Unstable axially symmetric mhd flow between rotating boundaries
|1Loginov, AA, 2Samoilenko, Yu.I, 1Tkachenko, VA |
1Space Research Institute of the National Academy of Sciences of Ukraine and the State Space Agency of Ukraine, Kyiv, Ukraine
2Institute of Mathematics, National Academy of Sciences of Ukraine, Kyiv, Ukraine
|Kosm. nauka tehnol. 2001, 7 ;(Suppl. 2):019-025|
|Section: Space and Atmospheric Physics|
|Publication Language: English|
For cylindrical and spherical liquid layers confined between two rotating axially symmetric shells the conditions for azimuth flow instability creating meridional component rise were obtained. Methods for solution of nonlinear equation describing steady-state flow for large Reynolds numbers were proposed.
1. Krechetov V. V. Tidal Forces Generation of Planetary Magnetic Fields. Space Res., 37 (4), 392—396 (1999) [in Russian]. e:EN-US'>7. Cornwall J. M. In: J. Geophys. Res., 77, 1756 (1972).