Zobrazeno 1 - 10
of 19
pro vyhledávání: '"Konishi, Takeharu"'
Autor:
Konishi, Takeharu, Chikawa, Michiyuki, Kato, Yukihiro, Kitamura, Takashi, Morizane, Yuichiro, Ohara, Soji, Tsuji, Katsufumi, yasui, Kenji
Publikováno v:
近畿大学理工学部研究報告 = Journal of the Faculty of Science and Engineering, Kinki University. 35:27-32
LAAS group (LAAS グループ)
A study of a phenomena deviated from random feature in EAS energy around 100TeV with new Kinki Array
Autor:
Chikawa, Michiyuki, Goya, Takeshi, Morizane, Yuichiro, Takama, Hiromitsu, Sakida, Shigekazu, Yasui, Kenji, Kato, Yukihiro, Kitamura, Takashi, Konishi, Takeharu, Tsujies, Katsufumi
Publikováno v:
理工学総合研究所研究報告 = Annual reports by Research Institute for Science and Technology. 11:49-57
[Abstract] An EAS observation system was rebuilt in July 1998 at Kinki University which consists of seven 0.25m2 plastic scintillators with fast PMTs. The system works well to detect EASs energy around 100TeV at sea level. In the observation of more
Publikováno v:
理工学総合研究所研究報告 = Annual reports by Research Institute for Science and Technology. 10:9-12
[Abstract] The observed number of background 5958±87 in 1036 days of the Kamiokande III measurement is not inconsistent with contribution of neutron flux generated in showers initiated by underground muons, whereas the contribution of atmospheric ν
Publikováno v:
理工学総合研究所研究報告 = Annual reports by Research Institute for Science and Technology. 10:13-19
[Abstract] We study the reconstruction resolution E[]1/2 of the arrival direction in the 8B neutrinos measurement by water Cherenkov detector and found the discrepancy with about 70% between the theoretical and experimental values for the root mean s
Autor:
CHIKAWA, Michiyuki, KITAMURA, Takashi, KONISHI, Takeharu, TSUJI, Katsufumi, KATO, Yukihiro, TAKAZAWA, Masaru, OHARA, Soji
Publikováno v:
理工学総合研究所研究報告 = Annual reports by Research Institute for Science and Technology. 9:59-64
[Abstract] We have reported a seriese of asearch for the directional analysis of EAS for the Kinki data concerning on the galactic coordinates with energy range between 10^ and 10^eV at sea level. In this report, I will present some basic results abo
Publikováno v:
理工学総合研究所研究報告 = Annual reports by Research Institute for Science and Technology. 9:25-28
[Abstract] The main background events seem to be caused by the low enegy atmospheric neutrinos. However, the events number can not interpleted by the expected numbers from the relevant cross sections ν_e+p→n+e^- and ν^^-_e+p→n+e^-. We show the
Autor:
Kitamura, Takashi, Chikawa, Michiyuki, Unno, Wasaburo, Tsuji, Katsufumi, Konishi, Takeharu, Ohara, Soji, Masaki, Isao
Publikováno v:
理工学総合研究所研究報告 = Annual reports by Research Institute for Science and Technology. 8:23-39
[Abstract] Unexpected chaotic features are found in time series of successive air shower (E>3×10^eV) arrival time intervals. Over 99.9 % of air shower arrival time intervals obey the Poisson distribution law representing stochastic behaviors, but th
Autor:
Ohara, Soji, Kitamura, Takashi, Chikawa, Michiyuki, Unno, Wasaburo, Tsuji, Katsufumi, Konishi, Takeharu, Masaki, Isao
Publikováno v:
理工学総合研究所研究報告 = Annual reports by Research Institute for Science and Technology. 7:39-46
[Abstract] The fractal dimensionality in time series of air shower arriving time intervals (ASATs) is observed for cosmic rays of energies larger than 3 × 10^ eV . We found 9 cases each composed of 128 ASATs for low fractal dimension (minimum 1.3) a
Publikováno v:
理工学総合研究所研究報告 = Annual reports by Research Institute for Science and Technology. 5:77-84
[Abstract] Extensive air showers have been observed with eight plastic scintillation counters since June 1991. The time structure of the air shower events is confirmed to follow a Poisson distribution. To search for air shower bursts, we have analyze
Publikováno v:
理工学総合研究所研究報告 = Annual reports by Research Institute for Science and Technology. 4:47-53
[Abstract] Using some statistical methods, many investigators have claimed on a basis of the polar angle "cos θ" distribution of neutrinos emitted from SN 1987A that the IMB data seem to be of a non-isotropic distribution, whereas the Kamiokande dat