MHD simulations of the magnetosheath

Details MHD simulations of the magnetosheath MHD simulations of the magnetosheath

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994adspr..14...21l&link_type=abstract

Advances in Space Research, Volume 14, Issue 7, p. 21-28.

Physics

7

Scientific paper

Ideal MHD simulations of the dayside magnetosheath are reported. The calculations show a depletion layer near the magnetopause and a new stagnation flow structure. The stagnation flow appears to be a generalization of the stagnation line for ideal MHD. For Mach numbers typical of the solar wind at the Earth, there is no evidence of the slow mode waves recently observed, but for low Mach numbers prominent slow mode waves are seen in the magnetosheath.

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