LISM Magnetic Field and Neutrals Effects on the Structure of the Heliospheric Boundary

Details LISM Magnetic Field and Neutrals Effects on the Structure of the Heliospheric Boundary LISM Magnetic Field and Neutrals Effects on the Structure of the Heliospheric Boundary

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sh31b03r&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SH31B-03

Physics

2164 Solar Wind Plasma, 7524 Magnetic Fields, 7811 Discontinuities, 7837 Neutral Particles, 7843 Numerical Simulation Studies

Scientific paper

In this paper we are using a sophisticated 3DT MHD+N model of the solar wind - interstellar medium interaction as a new diagnosis tool to constrain the structure of the heliospheric boundary region. This work is done to confront the model with measurements (HST, Voyagers, Ulysses etc.) in the future. We analyse several cases for different interstellar boundary conditions to see their effect on the heliosphere and the heliospheric interfaces. From about 90 calculated cases we have chosen the most characteristic and instructive. We present and discuss them in detail.

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