Physics
Scientist
Department of Physics, Yunnan University, China
Department of Physics, Hirosaki University, Hirosaki, Japan
Konan Univ., Kobe, Japan
Department of Physics, Hirosaki University, Hirosaki, JapanZ.CaoL. K.DingInstitute of High Energy Physics, Chinese Academy of Sciences, Beijing, ChinaZ. Y.FengDepartment of Physics, South West Jiaotong University, Chengdu, ChinaK.HibinoInstitute for Cosmic Ray Research, University of Tokyo, Tanashi, JapanN.HottaFaculty of Education, Utsunomiya University, Utsunomiya, JapanQ.HuangDepartment of Physics, South Jiaotong University, Chengdu, ChinaA. X.HuoInstitute of High Energy Physics, Chinese Academy of Sciences, Beijing, ChinaH. Y.JiaG. Z.JiangS. Q.JiaoDepartment of Physics, South West Jiaotong University, Chengdu, ChinaF.KajinoDepartment of Physics, Konan University, Kobe, JapanK.KasaharaFaculty of Engineering, Kanagawa University, Yokohama, JapanLabacirenD. M.MeiDepartment of Mathematics and Physics, Tibet Universityk Lhasa, ChinaL.MengInstitute of High Energy Physics, Chinese Academy of Sciences, Beijing, ChinaX. R.MengMimacirenDepartment of Mathematics and Physics, Tibet University, Lhasa, ChinaK.MizutaniDepartment of Physics, Saitama University, Urawa, JapanJ.MuDepartment of Physics, Yunnan University, Kunming, ChinaH.NanjoDepartment of Physics, Hirosaki University, Horosaki, JapanM.NishizawaDepartment of Physics, Konan University, Kobe, JapanNusangDepartment of Mathematics and Physics, Tibet University, Lhasa, ChinaA.OguroDepartment of Physics, Saitama University, Urawa, JapanM.OhnishiDepartment of Physics, Konan University, Kobe, JapanI.OhtaFaculty of Education, Utsunomiya University, Utsunomiya, JapanJ. R.RenInstitute of High Energy Physics, Chinese Academy of Sciences, Beijing, ChinaTo.SaitoInstitute for Cosmic Ray Research, University of Tokyo, Tanashi, JapanM.SakataDepartment of Physics, Konan University, Kobe, JapanZ. Z.ShiInstitute of High Energy Physics, Chinese Academy of Sciences, Beijing, ChinaM.ShibataFaculty of Education, Yokohama National University, Yokohama, Ja
A new project to search for high energy gamma ray point souces in Tibet
An analysis of primary cosmic-ray composition at energies around 10 to the 14th eV using single-shower events observed by mountain emulsion chamber
Behavior and Structure of Super-Families Observed with the Emulsion Chambers at Mts. Fuji and Kanbala
Big Family Events Observed at MT. Kanbala
Cosmic-ray deficit from the directions of the Moon and the Sun detected with the Tibet air-shower array
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