Solar wind composition signatures of coronal mass ejections

Details Solar wind composition signatures of coronal mass ejections Solar wind composition signatures of coronal mass ejections

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sh22c07r&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SH22C-07

Physics

2169 Sources Of The Solar Wind, 7509 Corona, 7513 Coronal Mass Ejections

Scientific paper

We present results from an analysis of CME ejecta detected at the ACE spacecraft between 1998 and 2000. The results indicate anomalous composition signatures of CMEs in both elemental and charge state composition. We discuss the anomalous elemental composition in the framework of elemental fractionation and magnetic field diffusion models. This analysis has important implications for understanding the origin and propogation of coronal mass ejections and the solar magnetic field regeneration.

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