Issue |
EPJ Web Conf.
Volume 210, 2019
Ultra High Energy Cosmic Rays 2018 (UHECR 2018)
|
|
---|---|---|
Article Number | 06004 | |
Number of page(s) | 7 | |
Section | Futur Detectors | |
DOI | https://doi.org/10.1051/epjconf/201921006004 | |
Published online | 17 May 2019 |
https://doi.org/10.1051/epjconf/201921006004
Detection of ultra-high energy cosmic ray air showers by Cosmic Ray Air Fluorescence Fresnel lens Telescope for next generation
1
Osaka Electro Communication University, Neyagawa, Osaka, Japan
2
Shinshu University, Nagano, Nagano, Japan
3
Earthquake Research Institute, University of Tokyo, Bunkyo-ku, Tokyo, Japan
4
Kanagawa University, Yokohama, Kanagawa, Japan
* e-mail: tameda@osakac.ac.jp
Published online: 17 May 2019
In the future, ultra-high energy cosmic ray (UHECR) observatory will be expanded due to the small flux. Then, cost reduction is useful strategy to realize a huge scale observatory. For this purpose, we are developing a simple structure cosmic ray detector named as Cosmic Ray Air Fluorescence Fresnel-lens Telescope (CRAFFT). We deployed CRAFFT detectors at the Telescope Array site and performed a test observation. We have successfully observed UHECR air showers. We will report the status and the result of the test observation.
© The Authors, published by EDP Sciences, 2019
This is an open access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.