Physics
Scientific paper
Dec 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011agufmsh53a2024b&link_type=abstract
American Geophysical Union, Fall Meeting 2011, abstract #SH53A-2024
Physics
[2101] Interplanetary Physics / Coronal Mass Ejections, [2124] Interplanetary Physics / Heliopause And Solar Wind Termination, [2164] Interplanetary Physics / Solar Wind Plasma
Scientific paper
We investigate the time-dependent propagation of 4 November 1997 CME in the heliosphere and through the termination shock into the heliosheath. The input plasma data were obtained at 10 Sun radii (Rs) from the Solar-InterPlanetary Conservation Element/Solution Element (SIP-CESE) MHD model. The data were propagated to 50Rs using the Multi-Scale Fluid Kinetic Simulation Suite (MS-FLUKSS) developed at the University of Alabama in Huntsville and compared with the output of the SIP-CESE MHD model. The results appear to be in a good agreement. Time-dependent data obtained at 50 Rs was used in global simulation of the interaction of the solar wind with the local interstellar medium. We show the effects of the CME evolution onto the heliospheric interface.
Borovikov Sergey N.
Feng Xue-Shang
Pogorelov Nikolai V.
Wu Seongho
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