Speaker
Prof.
Hiroshi Kojima
(Aichi Institute of Technology, Waterloo Road, Aichi, Japan)
Description
For the investigation of the interactions of galactic cosmic rays with the solar wind plasma and/or interplanetary magnetic field, it is important to know the rigidity dependence of the intensity variations of galactic cosmic rays in detail. In this paper, we have divided the data into two durations of active and calm by a criteria which is based on the data of neutron monitor of the lowest geomagnetic cut-off rigidity on the Earth.
Registration number following "ICRC2015-I/" | 171 |
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Collaboration | -- not specified -- |
Author
Prof.
Hiroshi Kojima
(Aichi Institute of Technology, Waterloo Road, Aichi, Japan)
Co-authors
Dr
Akitoshi Oshima
(Chubu University, Aichi, Japan)
Mr
Atul Jain
(Tata Institute of Fundamental Research, Mumbai, India)
Mr
B.S Rao
(Tata Institute of Fundamental Research, Mumbai, India)
Prof.
H.M Antia
(Tata Institute of Fundamental Research, Mumbai, India)
Prof.
Hisanori Takamaru
(Chubu University, Aichi, Japan)
Prof.
Isao Morishita
(Asahi University, Aichi, Japan)
Dr
Katsuya Yamazaki
(Osaka City University, Osaka, Japan)
Prof.
Koichi Tanaka
(Hiroshima City University, Hiroshima, Japan)
Prof.
Munetoshi Tokumaru
(Solar-Terrestrial Environment Laboratory, Nagoya University Furo-cho, Aichi, Japan)
Prof.
Nobuo Ito
(Osaka City University, Osaka, Japan)
Dr
P.K Mohanty
(Tata Institute of Fundamental Research, Mumbai, India)
Prof.
S.K Gupta
(Tata Institute of Fundamental Research, Mumbai, India)
Prof.
S.R Dugad
(Tata Institute of Fundamental Research, Mumbai, India)
Prof.
Saburo Kawakami
(Osaka City University, Osaka, Japan)
Prof.
Shoichi Ogio
(Osaka City University, Osaka, Japan)
Prof.
Shoichi Shibata
(Chubu University, Aichi, Japan)
Prof.
Toru Nakamura
(Kochi University, Kochi, Japan)
Mr
Toshio Matsuyama
(Osaka City University, Osaka, Japan)
Dr
Toshiyuki Nonaka
(Institute of Cosmic Ray Research, Chiba, Japan)
Prof.
Yoshio Hayashi
(Osaka City University, Osaka, Japan)