Physics
Scientific paper
Dec 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufmsh14a1690u&link_type=abstract
American Geophysical Union, Fall Meeting 2007, abstract #SH14A-1690
Physics
2102 Corotating Streams, 2149 Mhd Waves And Turbulence (2752, 6050, 7836), 2152 Pickup Ions, 2164 Solar Wind Plasma, 2169 Solar Wind Sources
Scientific paper
A fully three-dimensional MHD model is used to simulate the global steady-state structure of the solar corona and solar wind for a solar magnetic dipole tilted by 60 and 90° to the solar rotation axis. The model accounts for the energy and momentum addition from Alfvén waves in the region between the base of the corona and Earth's orbit and for the effects of interstellar pickup protons in the outer heliosphere (1-100~AU). We present simulation results on the evolution of the heliospheric current sheet and the corotating interaction regions with heliocentric distance and on the effects of pickup protons in this evolution.
Goldstein Michel L.
Usmanov Arcadi V.
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