Two-Dimensional Adaptive Code for Simulation of Astrophysical Magnetohydrodynamic Flows

Details Two-Dimensional Adaptive Code for Simulation of Astrophysical Magnetohydrodynamic Flows Two-Dimensional Adaptive Code for Simulation of Astrophysical Magnetohydrodynamic Flows

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003a%26at...22..321d&link_type=abstract

Astronomical and Astrophysical Transactions, vol. 22, Issue 3, p.321-324

Statistics

Computation

3

Scientific paper

Integrated adaptive mesh for simulations of two-dimensional (2D) self-gravitating, axially symmetric magnetohydrodynamic (MHD) flows in spherical coordinates is constructed and a new adaptive numerical 2D MHD code is developed. This code allows us to simulate efficiently the gravitational collapse of magnetized rotating protostellar clouds. Illustrative test computations are presented.

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