A relationship between the flare-associated X-ray ejection and the coronal mass ejection

Details A relationship between the flare-associated X-ray ejection and the coronal mass ejection A relationship between the flare-associated X-ray ejection and the coronal mass ejection

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..213t&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

Sun: Corona, Flares, Coronal Mass Ejections (Cmes), X-Rays, Gamma Rays

Scientific paper

The X1.2 flare occurred on 23 April 1998 approximately 13° behind the eastern solar limb. Its C2.0 precursor has been identified as a rapidly expanding system of magnetic loops that was well-observed by Yohkoh. Basic parameters of this ejection have been estimated based on images from the SXT telescope. The evolution of the X-ray ejection has been compared to a sequence of coronal mass ejection images obtained by the LASCO coronograph onboard SOHO. Evidences that the X-ray ejection is responsible for an additional acceleration of the CME have been presented.

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