On the Cherenkov light produced at several observatory altitudes by extensive air showers in the energy range 0.01-10 TeV

Details On the Cherenkov light produced at several observatory altitudes by extensive air showers in the energy range 0.01-10 TeV On the Cherenkov light produced at several observatory altitudes by extensive air showers in the energy range 0.01-10 TeV

Jan 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998jphg...24..235p&link_type=abstract

Journal of Physics G: Nuclear and Particle Physics, Volume 24, Issue 1, pp. 235-253 (1998).

Physics

4

Scientific paper

A Monte Carlo simulation of the development of atmospheric showers initiated by protons and 0954-3899/24/1/026/img1-rays in the energy range 0.01-10 TeV has been carried out. The features of the Cherenkov light component as expected at observatory depths ranging from 0954-3899/24/1/026/img2 up to sea level have been studied. The radial distribution of the Cherenkov light including a detailed description of the fluctuations will be shown. The dependence of the effective collection area of a Cherenkov telescope on both the primary energy and the observation altitude has been determined for several trigger conditions.

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