Performance of the Extensive Air Shower Array at the University of Puebla

Details Performance of the Extensive Air Shower Array at the University of Puebla Performance of the Extensive Air Shower Array at the University of Puebla

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....2.1017c&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

We report on the performance of the EAS-UAP extensive air shower array after one year of operation. The array is located at 19N 90W, 800 g /cm2 ; it was designed to measure the energy and arrival direction of primary cosmic rays with energies in the range of 1014 to 1016 eV. The array consists of 12 liquid scintillation detectors of 1m2 effective area distributed in a square grid of 20m that measure the lateral distribution function of the electromagnetic component and 3 large water Cherenkov detectors to help improve the measurement of the time profile of the signals.

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