G.S. Bisnovatyi-Kogan, S.G. Moiseenko, Rîbachin Boris, Secrieru Grigore
In the paper we describe the results of mathematical modelling of magnetorotational(MR) supernova explosion in 1D and 2D approach and formulate the problems and features for the numerical approach to simulations of the MR supernovae in 3D case.
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