The Heliosphere Interface in Different Models

Details The Heliosphere Interface in Different Models The Heliosphere Interface in Different Models

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsh21b1592g&link_type=abstract

American Geophysical Union, Fall Meeting 2008, abstract #SH21B-1592

Other

2104 Cosmic Rays, 2114 Energetic Particles (7514), 2124 Heliopause And Solar Wind Termination, 2126 Heliosphere/Interstellar Medium Interactions, 2162 Solar Cycle Variations (7536)

Scientific paper

In this paper results of modeling of the heliosphere interface obtained from the 3D MHD simulations are shown. We analyze heliosphere asymmetries for several sets of boundary conditions of the unperturbed solar wind and interstellar medium. Models are calculated for the spherical/non-spherical solar wind, and with/without the interplanetary magnetic field, in the presence of the interstellar magnetic field. The plasma - neutral hydrogen interaction via charge exchange is included. Comparison with other results is presented.

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