Do X-ray plasma ejections accelerate Coronal Mass Ejections?

Details Do X-ray plasma ejections accelerate Coronal Mass Ejections? Do X-ray plasma ejections accelerate Coronal Mass Ejections?

Apr 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004a%26a...417.1133t&link_type=abstract

Astronomy and Astrophysics, v.417, p.1133-1143 (2004)

Astronomy and Astrophysics

Astrophysics

2

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 is identified as a rapidly expanding system of magnetic loops that was well-observed by Yohkoh. Basic parameters of this ejection are estimated based on images from the SXT telescope. The evolution of the X-ray ejection is compared to a sequence of CME images obtained by the LASCO coronagraph onboard SOHO. Evidence that the X-ray ejection is responsible for an additional acceleration of the CME is presented. A possible scenario of the event is suggested.

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