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dc.contributor.authorPapaioannou, A.
dc.contributor.authorVainio, R.
dc.contributor.authorRaukunen, O.
dc.contributor.authorJiggens, P.
dc.contributor.authorAran, A.
dc.contributor.authorDierckxsens, M.
dc.contributor.authorMallios, S.A.
dc.contributor.authorPaassilta, M.
dc.contributor.authorAnastasiadis, A.
dc.date2022
dc.date.accessioned2022-06-28T15:31:13Z
dc.date.available2022-06-28T15:31:13Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/9988
dc.descriptionThe Probabilistic Solar Particle Event foRecasting (PROSPER) model predicts the probability of occurrence and the expected peak flux of solar energetic particle (SEP) events. Predictions are derived for a set of integral proton energies (i.e., E > 10, > 30, and > 100 MeV) from characteristics of solar flares (longitude, magnitude), coronal mass ejections (width, speed), and combinations of both. Herein the PROSPER model methodology for deriving the SEP event forecasts is described, and the validation of the model, based on archived data, is presented for a set of case studies. The PROSPER model has been incorporated into the new operational advanced solar particle event casting system (ASPECS) tool to provide nowcasting (short term forecasting) of SEP events as part of ESA’s future SEP advanced warning system (SAWS). ASPECS also provides the capability to interrogate PROSPER for historical cases via a run-on-demand functionality.
dc.languageeng
dc.titleThe probabilistic solar particle event forecasting (PROSPER) model
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freesolar flares
dc.subject.freecoronal mass ejections
dc.subject.freesolar energetic particles
dc.subject.freeoperational tool
dc.subject.freevalidation
dc.subject.freeradiation storms
dc.source.titleJournal of Space Weather and Space Climate
dc.source.volume12
dc.source.pageA24
Orfeo.peerreviewedYes
dc.identifier.doi10.1051/swsc/2022019
dc.identifier.scopus


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