Validating the proton prediction system (PPS)

Author: S.W. Kahler, E. W. Cliver and Alan G. Ling
Date: 
February 1, 2007
Type: 
Journal Article
Venue: 
Journal of Atmospheric and Solar-Terrestrial Physics
Citation: 

Kahler, S.W., E.W. Cliver, and A.G. Ling (2007), Validating the proton prediction system (PPS), Journal of Atmospheric and Solar-Terrestrial Physics 69, 43, doi:10.1016/j.jastp.2006.06.009

The proton prediction system (PPS) is a program developed at the Air Force Research Laboratory (AFRL) to predict solar energetic (E>5MeV) proton (SEP) intensities at 1 AU following solar flares. It is based on average observed SEP intensity-time profiles, peak intensities, and event durations. The input parameters are solar flare peak or time-integrated X-ray or radio fluxes and their times of onsets and maxima, and solar flare locations. We do a limited validation of the PPS using 78 GOES solar X-ray flares of peak intensity greater-or-equal,M5 with well associated Hα flare locations. Predicted peak proton intensities J((E>10MeV)) and event onset and rise times are compared with SEP events observed by GOES. We also select all GOES E>10MeV SEP events above 10 proton flux units (pfu) during the same time period to compare with those predicted by the PPS. With our M5 X-ray flare threshold the PPS yields approximately equal numbers of correct predictions, false predictions, and missed 10-pfu SEP events.