The Composition of Interplanetary Coronal Mass Ejections

Details The Composition of Interplanetary Coronal Mass Ejections The Composition of Interplanetary Coronal Mass Ejections

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679..604z&link_type=abstract

SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 604-6

Physics

4

Particle Emission, Solar Wind, Composition

Scientific paper

Interplanetary coronal mass ejection (ICME) associated plasma can exhibit signatures in elemental, ionic and isotopic composition. These signatures occur in less than 50% of all ICMEs, but are very indicative of ICME plasma. We review these compositional anomalies and briefly discuss a physical scenario that could be responsible for these anomalies.

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