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WP5: Gamma-ray, radio and SEP observations of relativistic events
This WP shall:
- Establish the link between relativistic protons in the solar atmosphere and near Earth in order to elucidate under which conditions protons and nucleons are accelerated at the Sun to such energies and if and how they escape to IP space
- Conduct multi-frequency observations of hard X-ray (HXR) and radio emissions in order to (i) constrain the relationship of gamma-ray emission with other electromagnetic signatures of energetic particles, (ii) obtain observational indications about the confinement or escape of particles accelerated in the low solar atmosphere, (iii) search for proxies of proton acceleration that can be used for forecasting purposes at times when no adequate gamma-ray detectors are available
