Exploring the CME-ICME Connection via CME Event Studies

Details Exploring the CME-ICME Connection via CME Event Studies Exploring the CME-ICME Connection via CME Event Studies

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agusmsp24a..06m&link_type=abstract

American Geophysical Union, Spring Meeting 2008, abstract #SP24A-06

Physics

2134 Interplanetary Magnetic Fields, 7509 Corona, 7513 Coronal Mass Ejections (2101), 7524 Magnetic Fields

Scientific paper

We describe how numerical simulations of CME initiation and propagation in the heliosphere can be used to study the connection between coronal mass ejections and interplanetary magnetic clouds. The detailed relationship between the plasma and magnetic fields in solar active regions, the source regions of CMEs, and subsequent in situ measurements in interplanetary magnetic clouds, can best be studied using "CME event studies." These attempt to model a particular CME in the greatest possible detail, including the use of measured photospheric magnetic fields, to explain observations. We will describe our event studies of the May 12, 1997 SHINE CME Event, as well as the May 13, 2005 LWS Focused Science Topic CME Event. Research supported by NASA's Living With a Star Program, NASA's Heliospheric Theory Program, and NSF/CISM.

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