Flare Probabilities [%] (00:00 UTC +24H) ?
NOAA C+ M+ X+ Mean ?
MCEVOL ? MCSTAT ? SWPC ? MCEVOL MCSTAT SWPC MCEVOL MCSTAT SWPC C+ M+ X+
13765 74 8 0 0 1 0 0 0 0 27 0 0
13767 74 8 - 0 1 - 0 0 - 41 0 0
13769 4 8 10 0 1 1 0 0 1 8 1 0
13770 39 15 0 0 2 0 0 0 0 18 1 0
13772 92 92 80 32 35 35 3 5 5 88 34 4
13774 92 92 80 32 35 35 3 5 10 88 34 6
13775 49 57 50 5 6 15 0 0 1 52 9 1
13777 11 22 30 1 2 10 0 0 1 21 5 0
13779 - 33 30 - 4 5 - 0 1 32 4 1
13780 - 57 90 - 6 50 - 0 15 74 28 8

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)