Development of the FNIT detector for 2-20 MeV solar neutrons

ORAL

Abstract

The Fast Neutron Imaging Telescope (FNIT) is a newly developed neutron detector with imaging and energy measurement capabilities, sensitive to neutrons in the 2-20 MeV energy range. FNIT was conceived as a candidate instrument for the Solar Sentinels program. Its design is optimized to measure neutrons produced in solar flares from the inner heliosphere. The detection principle is based on multiple elastic neutron-proton scatterings in plastic scintillators. By measuring the scattering coordinates and determining the energy of recoil protons and time of flight of scattered neutrons, the energy spectrum and incident direction of primary neutrons can be reconstructed. We present the results of recent laboratory efforts and describe the performance of the FNIT prototype.

Authors

  • Ulisse Bravar

  • Paul J. Bruillard

    University of New Hampshire

  • Erwin O. Flueckiger

    University of Bern

  • Alec L. MacKinnon

    University of Glasgow

  • John R. Macri

  • Mark McConnell

    University of New Hampshire

  • Michael R. Moser

    University of Bern

  • James M. Ryan

    University of New Hampshire