The objectives of HESPERIA are:

  • To develop two novel SEP forecasting systems based upon proven concepts.
  • To develop SEP forecasting tools searching for electromagnetic proxies of the gamma-ray emission in order to predict large SEP events.
  • To perform systematic exploitation of the novel high-energy gamma-ray observations of the FERMI mission together with in situ SEP measurements near 1 AU
  • To provide for the first time publicly available software to invert neutron monitor observations of relativistic SEPs to physical parameters that can be compared with the spaceborne measurements at lower energies.
  • To perform examination of currently unexploited tools (radio emission)
  • To design recommendations for future SEP forecasting systems.
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