Physics
Scientific paper
Sep 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008espm...12.2.96t&link_type=abstract
"12th European Solar Physics Meeting, Freiburg, Germany, held September, 8-12, 2008. Online at http://espm.kis.uni-freiburg.de/,
Physics
Scientific paper
In the standard flare/CME picture magnetic reconnection occurs in a current sheet formed behind the CME, which may provide a feedback relationship between both phenomena. To study the relationship of the large-scale CME acceleration and the energy release in the associated flare we analyze three well observed events. The observations cover the early (low corona) evolution of the CMEs with the EUVI instruments aboard the twin STEREO spacecraft and the RHESSI hard X-ray emission of the associated flare. Since the flare hard X-rays are due to fast electrons, they provide the most direct indicator of the evolution of the flare energy release in the flare. The results are compared to case studies for halo-CMEs where a close synchronization between the CME acceleration and the flare energy release was found (Temmer et al., ApJ, 2008, 673, L95).
Temmer Manuela
Veronig Astrid M.
Vrsnak Bojan
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