Gamma-ray detectors (greater than 10 MeV)

Details Gamma-ray detectors (greater than 10 MeV) Gamma-ray detectors (greater than 10 MeV)

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..118..291o&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 118, no. 1-2, 1988, p. 291-307.

Physics

2

Energetic Particles, Gamma Ray Spectrometers, High Energy Electrons, Solar Flares, Energy Spectra, Radiation Detectors, Satellite Instruments

Scientific paper

Photons in the energy region above 10 MeV can provide unique information about the highest energy particles produced in solar flares. Measurements of the energy spectra, temporal behavior and anisotropies of the incident photons, can give valuable insights into the particle acceleration process. Detection techniques used at these energies, typical instruments which use these techniques, and future solar missions both actual and potential are reviewed.

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