ESTIMATION OF THE RELIABILITY FUNCTION OF BASIC GOMPERTZ DISTRIBUTION UNDER DIFFERENT PRIORS



A time dependent relation between EUV solar flare light-curves from lines with differing formation temperatures

Extreme ultraviolet (EUV) solar flare emissions evolve in time as the emitting plasma heats and then cools.Although accurately modeling this evolution has been historically difficult, especially for empirical relationships, it is important for understanding processes at the Merchandising Sun, as well as for their influence on planetary atmospheres.

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