Abstract:
The numerical method for solution of the gravitational magnetogasdynamical equations has
been developed. The two-dimensional code for self-gravitating MHD-flows simulation on the
Eulerian cylindrical grid is constructed. This code is based on the explicit quasimonotonic
high resolution TVD-scheme. The results of test computations show that the code has a good
quality and can be applied to a wide class of plasma physics and astrophysics problems.