Heliospheric termination shock strength from a multi-fluid model

Details Heliospheric termination shock strength from a multi-fluid model Heliospheric termination shock strength from a multi-fluid model

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1039..384m&link_type=abstract

PARTICLE ACCELERATION AND TRANSPORT IN THE HELIOSPHERE AND BEYOND: 7th Annual International Astrophysics Conference. AIP Confer

Astronomy and Astrophysics

Astrophysics

2

Interstellar Medium And Nebulae In Milky Way, Plasma Temperature And Density, Planetary Bow Shocks, Interplanetary Shocks, Interplanetary Magnetic Fields, Particle Emission, Solar Wind, Flares, Abundances, Chemical Composition

Scientific paper

A suite of 64 global heliospheric models, for which the interstellar densities and temperatures are varied within reasonable bounds, is analyzed with respect to the location of the termination shock on and off the stagnation axis, its temperature, and its compression ratio. The empirical relations regarding the termination shock, the heliopause and the interstellar bow shock, are discussed, as are the physical reasons behind these relations.

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