The AVS-F experiment on recording rapidly changing fluxes of cosmic and gamma radiation prepared under the CORONAS-F project.

Details The AVS-F experiment on recording rapidly changing fluxes of cosmic and gamma radiation prepared under the CORONAS-F project. The AVS-F experiment on recording rapidly changing fluxes of cosmic and gamma radiation prepared under the CORONAS-F project.

Oct 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999iext...42..596g&link_type=abstract

Instrum. Exp. Tech., Vol. 42, No. 5, p. 596 - 603

Physics

Space Instrumentation: Solar X Rays, Space Instrumentation: Solar Gamma Rays

Scientific paper

The AVS-F instrumentation described is intended for recording fluxes of hard X-rays and γ-rays from the Sun in an energy range of 3 keV to 8 MeV aboard the CORONAS-F satellite. This system is expected to use detectors in the form of a CsI(Tl) scintillator and a nontraditional CdTe-based semiconductor detector, which would provide a higher than 1-keV resolution at a 5.9-keV energy level. Operation modes of the instrument are described and results of calculations are presented, which show that the device is capable of solving a new problem of recording fluxes of solar neutrons.

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