Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.148...85s&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 148, no. 1, Oct. 1988, p. 85-93.
Astronomy and Astrophysics
Astrophysics
2
Cylindrical Waves, Magnetohydrodynamics, Shock Waves, Density Distribution, Magnetic Fields, Shock Fronts, Velocity Distribution
Scientific paper
The Chester (1954, Chisnell (1955), and Whitham (1958) method has been used to investigate the propagation of converging and diverging cylindrical shock waves in a nonuniform medium under the influence of a magnetic field of constant strength. A comparison has also been made between the two types of cylindrical shock waves, simultaneously for both weak and strong cases of the magnetic field. The analytical expressions for shock velocity and shock strength as well as the pressure, the density, and the particle velocity just behind the shock front have been derived for both the cases.
Pandey Sudhir K.
~Singh ~B. J.
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