Linking remote and in-situ observations of Coronal Mass Ejections

Details Linking remote and in-situ observations of Coronal Mass Ejections Linking remote and in-situ observations of Coronal Mass Ejections

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agusmsh43a..03r&link_type=abstract

American Geophysical Union, Spring Meeting 2008, abstract #SH43A-03

Physics

2101 Coronal Mass Ejections (7513), 2111 Ejecta, Driver Gases, And Magnetic Clouds, 7519 Flares, 7924 Forecasting (2722), 7954 Magnetic Storms (2788)

Scientific paper

Providing connections between remote and in-situ observations of CMEs has the potential to offer insight into the evolution of CME plasma and magnetic structures during the transit to 1 AU, which can, in turn, inform models and improve predictions of CME properties. Progress has been made recently with statistical comparisons between ICME composition and plasma signatures and CME associated phenomena such as flare magnitude, source region location, and associated dimming region. These studies serve to strengthen the link between remote and in-situ observations. The results will be presented in the context of the large-scale structure of ICMEs and the contribution of associated phenomena to CME eruptions.

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