Flare Probabilities [%] (00:00 UTC +24H) ?
NOAA C+ M+ X+ Mean ?
MCEVOL ? MCSTAT ? SWPC ? MCEVOL MCSTAT SWPC MCEVOL MCSTAT SWPC C+ M+ X+
13922 22 33 30 22 4 5 0 0 1 29 10 0
13926 7 15 10 0 1 1 0 0 1 11 1 0
13927 - 8 10 - 1 1 - 0 1 9 1 1
13928 49 57 65 5 6 25 0 0 5 57 12 2
13929 9 5 5 0 0 1 0 0 1 6 0 0
13930 52 55 50 0 4 10 0 0 1 52 5 0
13931 8 9 5 0 0 1 0 0 1 7 1 0
13932 63 92 85 0 35 40 0 5 5 80 25 3
13933 - 33 45 - 4 15 - 0 5 39 9 3
13934 - 22 30 - 1 5 - 0 1 26 3 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)