Speaker
Atsushi Iyono
(Okayama University of Science)
Description
Observation experiments of Cosmic rays have been carried out since 1996
in Okayama University of Science, the primary energy spectrum in energy
range of 10^16eV to 10^19.5eV has been obtained by using a mini array
consist of 8 plastic scintillation counters and an extensive air shower
(EAS) time structure since 2006. And, in order to improve the energy
resolution of the mini array observation, data of zenith angle of EASs
have been collected since 2010.
In this presentation, we report on results of simulations and data
analysis for the primary energy estimate by taking account into primary
proton and iron nuclei, because primary particles had been assumed to be
proton nuclei in simulations and data analysis until 2013.
| Registration number following "ICRC2015-I/" | 299 |
|---|---|
| Collaboration | -- not specified -- |
Author
Co-authors
Atsushi Iyono
(Okayama University of Science)
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, Okayama University of Science)
Dr
SHUHEI TSUJI
(Kawasaki Medical School)
Prof.
SOJI OHARA
(Naragakuen University)
Prof.
TAKAO NAKATSUKA
(Okayama Shoka University)
