A global three dimensional hybrid simulation of the interaction between a weakly magnetized obstacle and the solar wind

Details A global three dimensional hybrid simulation of the interaction between a weakly magnetized obstacle and the solar wind A global three dimensional hybrid simulation of the interaction between a weakly magnetized obstacle and the solar wind

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679..485t&link_type=abstract

SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 485-4

Physics

Particle Emission, Solar Wind, Interplanetary Magnetic Fields, Heliopause And Solar Wind Termination, Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

We study an interaction between the solar wind flow and a conductive obstacle with a weak dipole magnetic field using a three dimensional implementation of the hybrid code. We show that the hybrid approach is capable of describing most of the structures formed due to the interaction between the solar wind and a magnetized planet like the bow shock, proton foreshock, magnetopause, magnetosheath, northern and southern cusps and the current sheath.

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