Understanding Interplanetary Coronal Mass Ejection Signatures. Report of Working Group B

Details Understanding Interplanetary Coronal Mass Ejection Signatures. Report of Working Group B Understanding Interplanetary Coronal Mass Ejection Signatures. Report of Working Group B

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ssrv..123..177w&link_type=abstract

Space Science Reviews, Volume 123, Issue 1-3, pp. 177-216

Physics

45

Coronal Mass Ejections, Interplanetary Physics, Solar Wind

Scientific paper

While interplanetary coronal mass ejections (ICMEs) are understood to be the heliospheric counterparts of CMEs, with signatures undeniably linked to the CME process, the variability of these signatures and questions about mapping to observed CME features raise issues that remain on the cutting edge of ICME research. These issues are discussed in the context of traditional understanding, and recent results using innovative analysis techniques are reviewed.

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