Flare Probabilities [%] (00:00 UTC +24H) ?
NOAA C+ M+ X+ Mean ?
MCEVOL ? MCSTAT ? SWPC ? MCEVOL MCSTAT SWPC MCEVOL MCSTAT SWPC C+ M+ X+
13806 42 44 15 5 4 1 0 0 1 34 3 0
13808 41 22 20 4 2 1 0 0 1 28 2 0
13811 - 39 20 - 2 5 - 0 1 29 3 0
13813 90 86 55 33 31 15 3 2 5 77 26 3
13814 8 15 20 1 2 5 0 0 1 14 3 0
13815 0 35 15 0 3 1 0 0 1 17 1 0
13816 9 5 15 0 0 1 0 0 1 10 1 0
13817 - 5 - - 0 - - 0 - 5 0 0
13818 - 22 15 - 2 1 - 0 1 19 2 0
13819 - 22 40 - 2 5 - 0 1 31 4 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)