Comparison of CME ejecta at 10 solar radii and 1 AU

Details Comparison of CME ejecta at 10 solar radii and 1 AU Comparison of CME ejecta at 10 solar radii and 1 AU

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agufmsh21a0493r&link_type=abstract

American Geophysical Union, Fall Meeting 2002, abstract #SH21A-0493

Physics

2164 Solar Wind Plasma, 2169 Sources Of The Solar Wind, 7513 Coronal Mass Ejections

Scientific paper

We present results from a study of CME composition profiles measured by the ACE spacecraft at 1 AU and extrapolated back to 10 solar radii based on the assumption of constant velocity. The results will be compared statistically to LASCO coronagraph CME observations on the limb to determine how CME density features are organized. We will attempt to determine a correspondence between visible CME density features such as leading edge, cavity, and prominence with features at 1 AU.

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