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- W111917966 abstract "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" @default.
- W111917966 created "2016-06-24" @default.
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- W111917966 date "1999-01-01" @default.
- W111917966 modified "2023-09-23" @default.
- W111917966 title "The Observed Spectral Evolution of Solar Flare Hard X-Ray Emission" @default.
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