Numerical simulation of shock waves in the heliosphere

Details Numerical simulation of shock waves in the heliosphere Numerical simulation of shock waves in the heliosphere

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991azh....68.1283k&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 68, Nov.-Dec. 1991, p. 1283-1298. In Russian.

Astronomy and Astrophysics

Astronomy

Coronal Loops, Digital Simulation, Heliosphere, Magnetohydrodynamics, Shock Wave Propagation, Solar Corona, Solar Wind, Approximation, Equations Of Motion, Finite Difference Theory, Magnetic Disturbances, Navier-Stokes Equation

Scientific paper

Results of calculations of shock waves generated by coronal transients and expanding flare loops are presented. The expanding magnetic loops act as a piston on the coronal plasma and produce shock waves propagating in the solar wind. The shock waves are computed in a 1D two-fluid approximation, taking turbulent dissipation processes into account. Shock wave parameters are obtained as functions of the initial perturbations of the magnetic loops.

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