HiRes/MIA Measurements of EAS Development Between 1017 and 1018eV:Detector description and Performance

Details HiRes/MIA Measurements of EAS Development Between 1017 and 1018eV:Detector description and Performance HiRes/MIA Measurements of EAS Development Between 1017 and 1018eV:Detector description and Performance

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999icrc....3..260a&link_type=abstract

Proceedings of the 26th International Cosmic Ray Conference. August 17-25, 1999. Salt Lake City, Utah, USA. Under the auspices o

Physics

Scientific paper

The HiRes prototype detector was operated for almost three years in coincidence with the CASA and MIA EAS arrays. We are able to extract mass composition information from the HiRes data (the shower depth of maximum) and from the MIA data (the muon content). In this paper we describe the detectors and their ability to measure mass composition parameters. Physics conclusions and their sensitivity to systematic effects are described in an accompanying paper (Abu-Zayyad et al. 1999).

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