Time variations of the 3D heliosphere over a solar cycle

Details Time variations of the 3D heliosphere over a solar cycle Time variations of the 3D heliosphere over a solar cycle

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1216..695g&link_type=abstract

TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP Conference Proceedings, Volume 1216, pp. 695-698 (2010).

Computer Science

1

Sunspots, Magnetohydrodynamics, Solar Magnetism, Solar Wind, Cosmic Rays, Sun Spots, Solar Cycles, Magnetohydrodynamics And Plasmas, Electric And Magnetic Fields, Solar Magnetism, Particle Emission, Solar Wind, Cosmic Rays

Scientific paper

The global structure of the heliosphere predicted from our 3D MHD time dependent code for several sets of boundary conditions is discussed. Time variations of the solar wind caused by the 11-year solar cycle are simulated, and the effect on the termination shock and heliopause is analyzed. The results from different models, assuming either spherical or anisotropic solar wind, with or without the interplanetary magnetic field, are compared. The interaction with neutral hydrogen via charge exchange is included. The role of the interstellar magnetic field is discussed.

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