Properties of Interplanetary Coronal Mass Ejections

Details Properties of Interplanetary Coronal Mass Ejections Properties of Interplanetary Coronal Mass Ejections

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ssrv..124..145g&link_type=abstract

Space Science Reviews, Volume 124, Issue 1-4, pp. 145-168

Physics

35

Coronal Mass Ejections, Interplanetary Cmes, Solar Wind, Magnetic Clouds, Shocks, Solar Flares, Geomagnetic Storms

Scientific paper

Interplanetary coronal mass ejections (ICMEs) originating from closed field regions on the Sun are the most energetic phenomenon in the heliosphere. They cause intense geomagnetic storms and drive fast mode shocks that accelerate charged particles. ICMEs are the interplanetary manifestations of CMEs typically remote-sensed by coronagraphs. This paper summarizes the observational properties of ICMEs with reference to the ordinary solar wind and the progenitor CMEs.

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