Sep 8 – 13, 2013
Asilomar, California
US/Pacific timezone

The mass composition of ultra-high energy cosmic rays measured by new fluorescence detectors in Telescope Array experiment

Sep 12, 2013, 5:00 PM
Asilomar, California

Asilomar, California

Asilomar Conference Grounds, 800 Asilomar Avenue, Pacific Grove, CA 93950-3704
Oral High-Energy Astrophysics (includes all cosmic ray physics) High Energy Astrophysics IV


Dr Toshihiro Fujii (University of Chicago)


The longitudinal development of an extensive air shower reaches its maximum at a depth, Xmax, that depends on the species of the primary cosmic ray. Using a technique based on Xmax, we measure the cosmic-ray mass composition from analyses of 3.7 years of monocular-mode operation of the newly constructed fluorescence detectors of the Telescope Array experiment.

Primary author

Dr Toshihiro Fujii (University of Chicago)

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