Influence of the interstellar magnetic field direction on the shape of the global heliopause

Details Influence of the interstellar magnetic field direction on the shape of the global heliopause Influence of the interstellar magnetic field direction on the shape of the global heliopause

Jan 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998jgr...103..237p&link_type=abstract

Journal of Geophysical Research, vol. 10, p. 237

Mathematics

48

Interstellar Magnetic Fields, Heliosphere, Magnetic Field Configurations, Solar Wind Velocity, Plasma Interactions, Vectors (Mathematics), Velocity Distribution, Supersonic Flow, Approximation, Shock Wave Interaction

Scientific paper

We study the influence of the angle between the local interstellar medium velocity and magnetic field vectors on the interaction of this medium with the solar wind. Both winds are supposed supersonic. The applicability of the two-shock model of the interaction is discussed. The investigation is performed by numerical solution of the MHD equations for an ideal plasma in the one-fluid approximation.

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