Flare Probabilities [%] (00:00 UTC +24H) ?
NOAA C+ M+ X+ Mean ?
MCEVOL ? MCSTAT ? SWPC ? MCEVOL MCSTAT SWPC MCEVOL MCSTAT SWPC C+ M+ X+
13792 12 19 0 0 1 0 0 0 0 10 0 0
13796 48 44 15 8 4 1 0 0 1 36 4 0
13798 4 8 5 0 1 1 0 0 1 6 1 0
13799 86 31 30 0 5 5 0 2 1 49 3 1
13800 72 68 65 12 9 30 0 0 5 68 17 2
13801 13 15 15 1 2 1 0 0 1 14 1 0
13802 9 5 - 0 0 - 0 0 - 7 0 0
13803 27 33 25 3 4 5 0 0 1 28 4 0
13804 4 8 5 0 1 1 0 0 1 6 1 0
13805 - 5 - - 0 - - 0 - 5 0 0
13806 - 33 35 - 4 15 - 0 5 34 9 3

SolarMonitor's flare prediction system's probabilities are calculated using the NOAA Space Weather Predicion Centre's McIntosh classifications. There are two methods, MCSTAT and MCEVOL, that use sunspot-group McIntosh classifications and Poisson statistics to calculate flaring probabilities valid for a 24-hr period starting at 00:00 UTC. The flaring probabilities are calculated using historical data from solar cycles 23 and 24 (1996-2019).

MCSTAT (McIntosh Statistics): Uses the point-in-time McIntosh classification to calculate Poisson flaring probabilities. Details about the method [1] and forecast verification testing [2] can be found in the following papers:

[1] Gallagher, P. T., Moon, Y.-J., Wang, H., Solar Physics, 209, 171, (2002)
[2] Bloomfield et al., 2012, The Astrophysical Journal Letters, 747, L41

MCEVOL (McIntosh Evolution): Uses a combination of previous and current McIntosh classification to calculate Poisson flaring probabilities. Details about the method and flaring rate statistics can be found in the following:

[1] McCloskey, A.E., Gallagher, P.T. & Bloomfield, D.S., Solar Physics, 291, 1711, (2016)