Speaker
Yuichiro Tameda
(Osaka Electro-Communication University)
Description
In order to obtain a sufficient number of observational events to clarify the origin of ultra high energy cosmic rays, a large-scale observatory is required. Currently, next-generation detectors are being developed for this purpose. The CRAFFT project focuses on developing fluorescence detectors that can be produced and operated at low cost. In this presentation, we will report on the status of detector upgrades, the development of trigger algorithms, and the operational tests of an observation system aimed at autonomous operation.
Primary author
Yuichiro Tameda
(Osaka Electro-Communication University)
