Three-dimensional MHD modeling of the solar wind with pick-up protons from the Sun to Voyagers 1 and 2

Details Three-dimensional MHD modeling of the solar wind with pick-up protons from the Sun to Voyagers 1 and 2 Three-dimensional MHD modeling of the solar wind with pick-up protons from the Sun to Voyagers 1 and 2

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsh21a1807d&link_type=abstract

American Geophysical Union, Fall Meeting 2010, abstract #SH21A-1807

Physics

Plasma Physics

[7514] Solar Physics, Astrophysics, And Astronomy / Energetic Particles, [7833] Space Plasma Physics / Mathematical And Numerical Techniques, [7837] Space Plasma Physics / Neutral Particles

Scientific paper

We have extended our 3D time-dependent magnetohydrodynamic (MHD) solar wind model, the Hybrid Heliospheric Modeling System with Pickup Protons (HHMS-PI) to to 100 AU. HHMS-PI (Detman et al., 2010) features a time-dependent lower boundary condition at 0.1 AU driven indirectly by solar observations via the Wang-Sheeley-Arge source surface current sheet model (Arge and Pizzo, 2000). We plan to compare preliminary results for solar wind and pickup protons with Voyagers 1 and 2 in the outer heliosphere. We consider the period beginning in May 2004.

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