Homothermal magnetogasdynamic shock waves caused by instantaneous monochromatic radiation

Details Homothermal magnetogasdynamic shock waves caused by instantaneous monochromatic radiation Homothermal magnetogasdynamic shock waves caused by instantaneous monochromatic radiation

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.103...27v&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 103, no. 1, Aug. 1984, p. 27-31.

Astronomy and Astrophysics

Astrophysics

Magnetohydrodynamic Waves, Monochromatic Radiation, Radiant Heating, Shock Waves, Differential Equations, Flow Equations, Magnetic Fields, Radiation Effects, Runge-Kutta Method, Spherical Waves

Scientific paper

Numerical solutions for the propagation of magnetogasdynamic shock waves caused by the action of instantaneous monochromatic radiation are obtained using the Runge-Kutta method. Boundary conditions at the shock surface are obtained, and variations of velocity, density, and magnetic field are graphically shown. It is concluded that these parameters increase for some distance from the shock surface toward the center of symmetry, but start to decrease after that.

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