Multiwavelength observations of the X-class flare of 25 August 2001

Details Multiwavelength observations of the X-class flare of 25 August 2001 Multiwavelength observations of the X-class flare of 25 August 2001

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..601f&link_type=abstract

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

Physics

2

Sun: Corona, Flares, X-Rays, Gamma Rays

Scientific paper

The X5.3 flare of 25 August 2001 was well-observed by the Yohkoh, SOHO and TRACE spacecraft. We analysed the Yohkoh hard and soft X-ray structures of this flare and compared them to SOHO and TRACE images. In hard X-rays we found two very bright footpoint sources and additionally a moving plasmoid-like feature with a projected velocity of about 450 km/s. This moving feature is observed up to 53-93 keV energies. We found evidences of this movement also in the TRACE and the EIT pictures with similar velocities.

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