Global Simulations of Propagating CMEs

Details Global Simulations of Propagating CMEs Global Simulations of Propagating CMEs

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agufmsh11d..06p&link_type=abstract

American Geophysical Union, Fall Meeting 2001, abstract #SH11D-06

Physics

2111 Ejecta, Driver Gases, And Magnetic Clouds, 2139 Interplanetary Shocks, 2164 Solar Wind Plasma, 3230 Numerical Solutions

Scientific paper

Recent advances in numerical methods and computer systems have made it possible to address complicated dynamic phenomena occurring in the heliosphere. Simulation of large-scale interplanetary interactions requires consideration of the preexisting structured ambient solar wind, realistic treatment of the launch phase of transient disturbances, and accurate tracking of interactions among multiple ambient and transient structures. We will review recent progress in this area, with special attention being given to the distortion of shocks and CMEs propagating within the streamer belt, to their possible appearance in in-situ and line-of-sight observations, and to phenomena generated by collisions of magnetic flux ropes and interplanetary shocks.

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