Three-dimensional structure of the outer heliosphere in the presence of the interstellar and interplanetary magnetic fields

Details Three-dimensional structure of the outer heliosphere in the presence of the interstellar and interplanetary magnetic fields Three-dimensional structure of the outer heliosphere in the presence of the interstellar and interplanetary magnetic fields

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..719...39p&link_type=abstract

PHYSICS OF THE OUTER HELIOSPHERE. AIP Conference Proceedings, Volume 719, pp. 39-46 (2004).

Physics

3

Particle Emission, Solar Wind, Interplanetary Magnetic Fields, Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

Three-dimensional structure of the heliosphere is analyzed for the effects of coupling between the interstellar and interplanetary magnetic fields (ISMF and IMF). The case when the ISMF is orthogonal to the velocity of the local interstellar medium, and tilted 60° to the ecliptic plane, is specifically investigated in view of the recent suggestion that this is the most probable ISMF orientation.

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