Speaker
Atsushi Iyono
(Okayama University of Science)
Description
In Large Area Air Shower experiments, one of EAS arrays is deployed on the second floor of four stories building in the campus of Okayama University of Science to limit the zenith angle acceptance of muon detection. This system provide EAS muon intensities from zenith solid angles. To compare these intensities with solar activities such as flares, CME and magnetic-storms, LAAS data have been analyzed. Faster data acquisition with Ha/CaK solar telescope have also been carried out. In this presentation, cosmic ray variations for four years since 2011 are going to be reported as well as fast image data.
Registration number following "ICRC2015-I/" | 299 |
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Collaboration | -- not specified -- |
Author
Mr
NAOKI WADA
(Graduate School of Science, Okayama University of Science)
Co-authors
Atsushi Iyono
(Okayama University of Science)
Hiroki Matsumoto
Prof.
Isao YAMAMOTO
(Okayama University of Science)
Dr
Kazuhide OKEI
(Kawasaki Medical School)
Dr
Nobuaki OCHI
(Toyo University)
Dr
Nobusuke TAKAHASHI
(Hirosaki University)
Ms
Saya YAMAMOTO
(Graduate School of Science, Okayama University of Science)
Dr
Shuhei TSUJI
(Kawasaki Medical School)
Prof.
Soji OHARA
(Naragakuen University)
Prof.
Takao NAKATSUKA
(Okayama Shoka University)