Flare Probabilities [%] (00:00 UTC +24H) ?
NOAA C+ M+ X+ Mean ?
MCEVOL ? MCSTAT ? SWPC ? MCEVOL MCSTAT SWPC MCEVOL MCSTAT SWPC C+ M+ X+
13784 92 86 80 52 35 30 6 6 5 86 39 6
13785 34 64 35 5 11 5 0 1 1 44 7 1
13786 10 8 0 1 1 0 0 0 0 6 0 0
13788 13 15 25 1 2 1 0 0 1 18 1 0
13789 36 57 10 5 6 1 0 0 1 35 4 0
13790 48 44 50 8 4 10 0 0 1 47 7 0
13791 26 9 10 2 0 1 0 0 1 15 1 0
13792 4 8 20 0 1 1 0 0 1 11 1 0
13793 - 27 25 - 3 1 - 0 1 26 2 1
13794 - 15 15 - 1 1 - 0 1 15 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)