Speaker
Dr
Masato TAKITA
(ICRR, the University of Tokyo)
Description
The Tibet air shower array is located at 4,300 m above sea level, Tibet, China.
In 2014, an array of underground muon detectors is added under the surface
air shower array. We would like to present recent results from the Tibet
ASgamma experiment on cosmic ray anisotropy, Sun shadow, and gamma-ray observation, together with some related topics.
Primary authors
Dr
Masato TAKITA
(ICRR, the University of Tokyo)
The Tibet ASgamma collaboration
