Table 2.
Comparison between BTL and on-disk LAT flares.
| Flare | Rise time | ΔPeak | Peak flux | AR |
|---|---|---|---|---|
| (min:s) | (s) | (10−5 ph cm−2 s−1) | ||
| SOL2013-10-11 | 9 : 00 ± 1 : 00 | 600 ± 60 | 49 ± 2 | N21E103 |
| SOL2014-09-01 | 9 : 00 ± 1 : 00 | 240 ± 60 | 565 ± 21 | N14E126 |
| SOL2021-07-17 | 8 : 00 ± 1 : 00 | – | 4 ± 1 | S20E140 |
| SOL2021-09-17 | 1 : 09 ± 0 : 07 | 189 ± 7 | 67 ± 20 | S30E100 |
| SOL2022-09-29 | 0 : 18 ± 0 : 04 | 5 ± 4 | 44 ± 14 | N26E106 |
| SOL2011-09-06 | 0 : 16 ± 0 : 01 | 10 ± 1 | 50 ± 16 | N14W18 |
Notes. Rise time, difference between GBM 32–76 keV and > 100 MeV peak times (ΔPeak), peak flux value of the gamma-ray emission, and the position of the active region for the five BTL flares detected with the LAT and with sufficient statistics to perform a time-resolved analysis (top table) and the impulsive on-disk flare of September 6, 2011 (bottom table). The criteria for the selection of the on-disk flare is described in the text. The BTL flare that is not considered here is the flare of January 6, 2014, due to a lack of sufficient coverage by the LAT. We do not list the value of ΔPeak for SOL2021-07-17 because the GBM did not detect any significant emission from this event.
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