Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993exa.....4...59l&link_type=abstract
Experimental Astronomy (ISSN 0922-6435), vol. 4, no. 1, p. 59-75
Astronomy and Astrophysics
Astronomy
Astronomical Satellites, Control Systems Design, Experiment Design, High Energy Interactions, Monitors, Off-On Control, Proton Damage, Radiation Belts, Radiation Detectors, Satellite Instruments, Spaceborne Experiments, Diodes, Electrons, Linear Accelerators, P-I-N Junctions, Photons, Protons
Scientific paper
A Radiation Belt Monitor (RBM) sensitive to protons and electrons with energy approximately greater than 0.5 MeV has been designed for the High Energy Transient Experiment (HETE) satellite in order to: first, control the on-off configuration of the experiments (i.e. those susceptible to proton damage); and second, to indicate the presence of proton and/or electron events that could masquerade as legitimate high energy photon events. One of the two RBM channels has an enhanced sensitivity to electrons. Each channel of the RBM, based on a PIN silicon diode, requires a typical power of 6 milliwatts. Tests have been performed with protons with energies from approximately 0.1 to 2.5 MeV (generated by a Cockcroft-Walton linear accelerator via the d(d,p)t reaction), and with electrons with energies up to 1 MeV (from a 1.0 microcurie Bi-207 source).
Doty John
Lo D. H.
Petrasso Richard D.
Prigozhin Gregory Y.
Ricker George
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