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1. • There are two kinds of outputs extracted from the flare association algorithm as follows:

     1. GOES magnitudes of all the associated flares

        • The GOES flare magnitude is written in the following format: e.g.,

        M1

        • C3.5=3.5,

        C3.4

        • M5.5=55.0, & X1.6=160.0

        • Note that B-class flares are not considered because they are in the range of the solar soft X-ray background level.

     2. Time differences between the SHARP observation time t₀ and start/peak/end times (t_s, t_p, t_e) of all the associated flares (units: in seconds)

        • t_s - t₀

        • t_p - t₀

        • t_e - t₀

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