Speaker
Dr
Toshihiro Fujii
(University of Chicago)
Description
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)
