TA Anisotropy Summary
The Telescope Array (TA) is the largest ultra-high-energy cosmic-ray (UHECR) detector in the northern hemisphere. It consists of an array of 507 surface detectors (SD) covering a total 700 km^2 and three fluorescence detector stations overlooking the SD array. In this proceedings, we summarize recent results on the search for directional anisotropy of UHECRs using the latest dataset collected by the TA SD array. We obtained hints of the anisotropy of the UHECRs in the northern sky from the various analyses.
2019
2020-04-27 23:45:47
1033
cosmic radiation, UHE detector, fluorescence detector, surface,Telescope Array Experiment, anisotropy, experimental results
r6
K.
Kawata
70
Jon Paul
Lundquist
70
COBISS_ID
3
12877059
DOI
15
10.1051/epjconf/201921001004
NUK URN
18
URN:SI:UNG:REP:0PGHPGPK
epjconf_uhecr18_01004.pdf
1972848
Predstavitvena datoteka
2020-04-27 23:45:56
0
Izvorni URL
2020-04-27 23:45:50