Investigating the Possibility of Associations between X-Ray Spectral Evolution and Eruptive Phenomena

Details Investigating the Possibility of Associations between X-Ray Spectral Evolution and Eruptive Phenomena Investigating the Possibility of Associations between X-Ray Spectral Evolution and Eruptive Phenomena

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000spd....31.0251n&link_type=abstract

American Astronomical Society, SPD Meeting #31, #02.51; Bulletin of the American Astronomical Society, Vol. 32, p.820

Astronomy and Astrophysics

Astronomy

Scientific paper

In previous investigations, we found consistent patterns of spectral evolution in the >30 keV hard X-rays emitted during solar flares. The characteristics of the observed spectral evolution support the idea that the particle acceleration mechanism is responsible for modulating the X-ray spectra in time and energy, rather than time-of-flight effects and trapping time differences. We report on a preliminary study of spectral evolution in flares associated with coronal mass ejections. Our interest lies in determining whether a given pattern of spectral evolution can be correlated with eruptive phenomena.

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