Measurement of solar hard X-ray emission

Details Measurement of solar hard X-ray emission Measurement of solar hard X-ray emission

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981izssr..45.1159b&link_type=abstract

(Evropeiskii Simpozium po Kosmicheskim Lucham, 7th, Leningrad, USSR, Sept. 15-19, 1980.) Akademiia Nauk SSSR, Izvestiia, Seriia

Astronomy and Astrophysics

Astronomy

Prognoz Satellites, Radiation Detectors, Solar Flares, Solar Radiation, X Ray Astronomy, X Ray Spectroscopy, Background Radiation, Radiant Flux Density, Satellite Observation, Sensitivity, Solar Activity Effects

Scientific paper

Characteristics of hard X-ray spectrometers used on the Prognoz satellites are discussed. These instruments feature a sensitivity of up to 10 to the -7th erg/sq cm s in the range 20-100 keV, a time resolution of 60 ms, and a wide energy range (2-100 keV). Hard X-ray emission bursts recorded during the period from Oct. 24 to Nov. 15, 1977 are presented.

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