Other
Scientific paper
May 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agusmsh31c..01l&link_type=abstract
American Geophysical Union, Spring Meeting 2008, abstract #SH31C-01
Other
7974 Solar Effects
Scientific paper
Models developed under the Center for Integrated Space weather Modeling (CISM) represent one effort that is underway to realistically simulate the Sun's physical controls over interplanetary conditions, or heliospheric "space weather", in three dimensions. This capability is critical for interpreting the latest observations from STEREO, whose goal is to enable connections to be made between what is observed in the heliosphere via distributed in-situ measurements and what is observed in the corona and heliosphere via imaging from separated 1 AU perspectives. The ways in which the CISM models are enabling the exploitation of STEREO and other observations toward increased understanding of the solar wind and coronal activity and its consequences are described. In particular, the models allow the identification of the sources of structures in the solar wind, and analyses of how the coronal context of the observed CMEs plays a key role in determining the ultimate terrestrial (and other planetary) response .
Arge Charles
Galvin Antoinette
Hoeksema Todd
Howard Ralph
Huttunen E.
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