Self-similar flows behind M.H.D. shock waves

Details Self-similar flows behind M.H.D. shock waves Self-similar flows behind M.H.D. shock waves

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.161..339r&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 161, no. 2, Nov. 1989, p. 339-345. Research supported by UGCI.

Statistics

Computation

Electrical Resistivity, Magnetic Fields, Magnetohydrodynamic Flow, Shock Fronts, Shock Waves, Space Plasmas, Boundary Value Problems, Computational Astrophysics, Numerical Integration, Runge-Kutta Method

Scientific paper

In this paper a self-similar motion in a medium of infinite electrical
conductivity has been investigated in spherical symmetry under the
influence of an idealized magnetic field and a comparison has been made
of the state of flow variables with and without magnetic field.

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