Computer Science
Scientific paper
Aug 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....6..133t&link_type=abstract
IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Conference Papers. Volume 6 (A85-2
Computer Science
Cosmic Ray Showers, Electrons, High Energy Interactions, Muons, Arrivals, Particle Size Distribution, Scintillation Counters, Time Response
Scientific paper
Arrival-time distributions of muons with E(mu) greater than 1 GeV in air showers with electron sizes from 10 to the 6.5th to 10 to the 8th have been studied at the Akeno air-shower array (930 g/sq cm atmospheric depth, 900 m above sea level) with four 4-sq-m scintillation detectors and a 100-MHz storage oscilloscope. The time response of the whole system to a single muon is 4.3 ns and 8.1 ns in rise time and FWHM, respectively. The median rise times between 20 and 70 percent of the integrated full-muon signal are compared with those expected from various models of high-energy particle interactions. Also described is a new observation on arrival-time distributions of muons and those of electrons at large core distances in air showers with electron sizes above 5 x 10 to the 8th.
Enoki Toshiaki
Inoue Naoya
Kakimoto Fumio
Matsumoto Yosuke
Nakatani Hitoshi
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