SPEARHEAD focuses on high energy particles, originating either from the Sun (i.e. Solar Energetic Particles – SEPs) or our Galaxy (Galactic Cosmic Rays – GCRs). The project will address several open scientific questions on the acceleration, release and propagation physical processes of such particles. In doing so, SPEARHEAD provides novel high-level data products based on recalibrations of radiation monitor data -- on so-far unreleased data from science-grade instruments, and measurements of ground-based neutron monitors; technical notes on the response functions of several science-grade and monitoring instruments, utilising GEANT4 modelling; comprehensive catalogues of near-relativistic ions and relativistic electrons in strong SEP (and/or Ground Level Enhancement - GLE) events as well as Forbush decreases - FD events of GCRs from a fleet of different instruments onboard spacecraft, at radial distances from 0.04 to 5 AU; scientific and data analysis as well as tools enabling the coordinated analysis of high energy particle data with contexts observations.
SPEARHEAD plans to leverage very-high-energy particle observations from the most important heliophysics missions and ground-based measurements to answer key questions related to particles and solar eruptions. The project will develop innovative solutions to derive high-energy particle fluxes from observations, improve the use of monitoring data and enhance the analysis of solar eruptions.