Measurement of UHECR composition by TA

Details Measurement of UHECR composition by TA Measurement of UHECR composition by TA

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aipc.1367..110t&link_type=abstract

INTERNATIONAL SYMPOSIUM ON THE RECENT PROGRESS OF ULTRA-HIGH ENERGY COSMIC RAY OBSERVATION. AIP Conference Proceedings, Volume

Statistics

Applications

Telescopes, Mass, Intergalactic Magnetic Fields, Monte Carlo Methods, Neutrino, Muon, Pion, And Other Elementary Particle Detectors, Cosmic Ray Detectors, Masses And Mass Distribution, Electric And Magnetic Fields, Applications Of Monte Carlo Methods

Scientific paper

The Telescope Array is a hybrid detector consisting of Fluorescence Detectors (FDs) and Surface Detectors (SDs) to observe ultra high energy cosmic rays (UHECRs). FDs are telescopes which can observe longitudinal developments of cosmic-ray air showers which strongly depend on their primary particle types. Especially Xmax is one of the most efficient parameter of shower development for cosmic-ray primary particle type. In this paper, the analysis framework for TA FD and the recent result of measurement of UHECR composition by TA FD stereo events is reported.

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