The Arrival Time Distribution far from the Core of Air Showers above 1018 eV Measured in AGASA

Details The Arrival Time Distribution far from the Core of Air Showers above 1018 eV Measured in AGASA The Arrival Time Distribution far from the Core of Air Showers above 1018 eV Measured in AGASA

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....1..361h&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

In order to know the arrival time of electrons and muons far from the cores of giant air showers, a detector with two scintillators sandwiching a lead plate of 1 cm thickness (Leadburger) has been built and placed at one corner of the Akeno Giant Air Shower Array (AGASA). The arrival time distributions of each component around 1000 m 2000 m from the core of showers with energies lager than 1018.5 eV are reported from data collected over 7 years. These data are compared with the results of the simulation.

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