Probing The Three Dimensional Structure Of Coronal Mass Ejections

Details Probing The Three Dimensional Structure Of Coronal Mass Ejections Probing The Three Dimensional Structure Of Coronal Mass Ejections

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009spd....40.2208r&link_type=abstract

American Astronomical Society, SPD meeting #40, #22.08; Bulletin of the American Astronomical Society, Vol. 41, p.859

Astronomy and Astrophysics

Astronomy

Scientific paper

The underlying causes of CMEs are not well understood, nor are the precise details of their internal magnetic and plasma structure. To fully understand the initiation and propagation of CME ejecta it is necessary to examine the full three-dimensional structure of ICME ejecta and to relate those in-situ structures to conditions at the solar source region. We use a non-cylindrical, non-force-free model along with spatial mapping techniques to probe the overall heliospheric ICME structure and provide a context for ACE and STEREO measurements of composition and plasma parameters. We report on the progress of this effort as applied to the ICMEs seen by ACE and STEREO on May 2007 and November 2007.

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