HESPERIA will build a real-time prediction tool for high-energy solar energetic particles (> 500 MeV) based on the UMASEP system (Nunez, 2011) by analyzing 1-min GOES X-ray flux, proton data, and neutron monitor data.

HESPERIA will build a real-time tool for predicting 30−50 MeV SEP events based on the RELeASE scheme (Posner 2007). The new aspect here is that the continuous set of near relativistic electron measurements by ACE/EPAM will be utilized for the first time to infer proton time profiles at 30−50 MeV.

Our website is protected by DMC Firewall!