The Observed Spectral Evolution of Solar Flare Hard X-Ray Emission

Details The Observed Spectral Evolution of Solar Flare Hard X-Ray Emission The Observed Spectral Evolution of Solar Flare Hard X-Ray Emission

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...194.8010n&link_type=abstract

American Astronomical Society, 194th AAS Meeting, #80.10; Bulletin of the American Astronomical Society, Vol. 31, p.966

Astronomy and Astrophysics

Astrophysics

Scientific paper

The spectral evolution of flare emission may be characterized using color-color diagrams (CCDs), a technique which has been widely employed by the astrophysics community, but not yet by the solar flare community. CCDs are constructed for a sample of flares observed simultaneously by CGRO/BATSE and Yohkoh/HXT. It is found that flare spectral evolution follows one of only a few patterns, which generally evolve differently than the soft-hard-soft pattern put forth as the norm in previous work. The implications for the nature of flare energy release and acceleration/propagation models are discussed.

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