Toward Routine Simulations of Heliospheric Transient Disturbances

Details Toward Routine Simulations of Heliospheric Transient Disturbances Toward Routine Simulations of Heliospheric Transient Disturbances

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufmsh53c..05o&link_type=abstract

American Geophysical Union, Fall Meeting 2006, abstract #SH53C-05

Physics

2101 Coronal Mass Ejections (7513), 2102 Corotating Streams, 2134 Interplanetary Magnetic Fields, 2164 Solar Wind Plasma

Scientific paper

The upcoming STEREO and SENTINELS missions will provide observations of heliospheric disturbances from multiple points yielding unprecedented clues to their 3D structure in the heliosphere. Routine and reliable 3D MHD heliospheric simulations are absolutely necessary for interpreting remote and in-situ observations. Since the MHD models of coronal mass ejections (CMEs) initiations are very distinctly in the research phase, an approach that relies upon parameterization of already formed CMEs, but which is based upon actual observations, is currently the only way to provide a routine and reliable simulation capability. We will present our recent results in application of this technique to observed events and show its advantages and limitations.

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