Flare Probabilities [%] (00:00 UTC +24H) ?
NOAA C+ M+ X+ Mean ?
MCEVOL ? MCSTAT ? SWPC ? MCEVOL MCSTAT SWPC MCEVOL MCSTAT SWPC C+ M+ X+
13784 87 86 60 37 35 20 9 6 5 78 31 7
13785 74 22 5 6 2 1 0 0 1 34 3 0
13788 4 8 5 0 1 1 0 0 1 6 1 0
13789 52 55 20 0 4 5 0 0 1 42 3 0
13790 87 86 70 37 35 25 9 6 5 81 33 7
13792 32 31 30 0 5 5 0 2 1 31 3 1
13793 27 33 5 3 4 1 0 0 1 22 3 0
13794 33 57 45 1 6 10 0 0 1 45 6 0
13796 76 77 70 10 18 25 0 1 5 75 18 2
13797 63 33 5 7 4 1 0 0 1 34 4 0
13798 4 8 5 0 1 1 0 0 1 6 1 0

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)