Analysis of Cerenkov burst data recorded by the GT-48 twin telescope

Details Analysis of Cerenkov burst data recorded by the GT-48 twin telescope Analysis of Cerenkov burst data recorded by the GT-48 twin telescope

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993roizf..57..158k&link_type=abstract

Rossijskaya Akademiya Nauk, Izvestiya, Seriya Fizicheskaya (ISSN 0367-6765), vol. 57, no. 4, p. 158-161.

Other

Cerenkov Radiation, Cosmic Ray Showers, Energetic Particles, Correlation Coefficients, Gamma Ray Telescopes

Scientific paper

The Cerenkov radiation bursts of extensive air showers were observed using the twin detectors of the GT-48 gamma telescope of the Crimean Astrophysical Observatory. The parallel detectors are spaced 20 m apart; the mean count rate of one detector was 35 percent higher than that of the other. A comparison between the parameters of the recorded bursts demonstrates good correlation between the locations of the burst centroids (r = 0.98), burst image lengths (r = 0.70), and orientation angles (r = 0.64). The correlation is weaker for the burst image widths (r = 0.44).

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