Flare Probabilities [%] (00:00 UTC +24H) ?
NOAA C+ M+ X+ Mean ?
MCEVOL ? MCSTAT ? SWPC ? MCEVOL MCSTAT SWPC MCEVOL MCSTAT SWPC C+ M+ X+
13836 12 9 - 0 0 - 0 0 - 10 0 0
13839 10 8 10 1 1 1 0 0 1 9 1 0
13841 49 57 50 5 6 15 0 0 1 52 9 1
13842 92 92 90 32 35 60 3 5 30 91 42 13
13843 - 68 45 - 9 15 - 0 1 57 12 0
13844 65 73 80 0 15 40 0 4 15 73 18 6
13845 9 5 5 0 0 1 0 0 1 6 1 0
13846 12 14 - 0 1 - 0 0 - 13 1 0
13847 4 10 5 0 0 1 0 0 1 6 0 0
13848 78 86 70 22 35 35 0 6 10 78 31 5

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)