Relating heliospheric CME composition and associated flare magnitude

Details Relating heliospheric CME composition and associated flare magnitude Relating heliospheric CME composition and associated flare magnitude

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsp44a..06r&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #SP44A-06

Physics

2111 Ejecta, Driver Gases, And Magnetic Clouds, 2139 Interplanetary Shocks, 2164 Solar Wind Plasma, 7513 Coronal Mass Ejections, 7519 Flares

Scientific paper

We present results from a continuing effort to study heliospheric CME ejecta within the context of solar CME observations. Previously we reported that in situ charge state ratios are positively correlated with associated flare magnitude for events occurring in central longitudes. We now present further correlations with elemental abundances of helium, neon and magnesium. We use partial correlation analysis to isolate the individual contributions from each signature. These correlations between in situ quantities and flare magnitudes indicate that flare eruptions have a stronger influence on CME material than previously thought.

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