Flare Probabilities [%] (00:00 UTC +24H) ?
NOAA ? C+ M+ X+ Mean ?
MCEVOL ? MCSTAT ? SWPC ? MCEVOL MCSTAT SWPC MCEVOL MCSTAT SWPC C+ M+ X+
14191 32 39 35 3 2 5 0 0 1 35 3 0
14197 92 92 75 32 35 35 3 5 15 86 34 8
14199 52 55 50 0 4 10 0 0 1 52 5 0
14200 22 27 25 2 3 5 0 0 1 25 3 0
14201 22 27 10 2 3 1 0 0 1 20 2 0
14202 7 15 10 0 1 1 0 0 1 11 1 0
14205 7 8 10 0 1 1 0 0 1 8 1 0
14206 4 8 10 0 1 1 0 0 1 8 1 0
14207 0 42 45 0 8 10 0 0 1 29 6 0
14208 - 22 20 - 1 5 - 0 1 21 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)