Comparison of 2-dimensional MHD and semiempirical models of interplanetary shock wave propagation

Details Comparison of 2-dimensional MHD and semiempirical models of interplanetary shock wave propagation Comparison of 2-dimensional MHD and semiempirical models of interplanetary shock wave propagation

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991baicz..42..320k&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 42, no. 5, Oct. 1991, p. 320-328.

Astronomy and Astrophysics

Astronomy

1

Astronomical Models, Interplanetary Medium, Magnetohydrodynamic Waves, Semiempirical Equations, Shock Wave Propagation, Boundary Value Problems, Mathematical Models, Shock Wave Profiles, Solar Wind

Scientific paper

A comparison was made between the 2D version of the 2 1/2-D MHD model by Wu et al.(1983) and the semiempirical model of Voros and Karlicky (1988). Although agreement in the exponential dependence (N is about 0.5) of shock wave velocities was found, the compared models differ in the early stages of shock wave propagation and in the shock shapes. A small E-W asymmetry of shock wave propagation was found in the MHD simulations.

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