Sensitivity of leakage neutrons to the abundance and depth distribution of lunar subsurface water

Autor: Kusano, Hiroki, Nagaoka, Hiroshi, Enoto, Teruaki, Yamashita, Naoyuki, Karouji, Yuzuru, Hoshino, Takeshi, Ueno, Munetaka, Hareyama, Makoto

Publikováno v: In Planetary and Space Science 15 October 2024 251

Are Galactic Cosmic Rays Accelerated inside the Ejectae Expanding just after Supernova Explosions ?

Autor: Hasebe, Nobuyuki, Hareyama, Makoto, Kodaira, Satoshi, Sakurai, Kunitomo

Publikováno v: In Nuclear Physics, Section A 2005 758:292-295

Estimation method of planetary fast neutron flux by a Ge gamma-ray spectrometer

Autor: Fujibayashi, Y., Yamashita, Y., Reedy, R. C., Gasnault, O., Forni, O., d'Uston, C., Kim, K. J., Hareyama, Makoto, Karouji, Yuzuru, Nagaoka, Hiroshi, Kobayashi, Shingo, Hasebe, Nobuyuki

Publikováno v: Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 828:145-155

著者人数: 12名
Accepted: 2016-05-10
資料番号: SA1160141000

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8a09799407cad1b4256f0597b87c5055
https://doi.org/10.1016/j.nima.2016.05.045

Energy Spectrum of Cosmic-Ray Electron and Positron from 10 GeV to 3 TeV Observed with the Calorimetric Electron Telescope on the International Space Station

Autor: CALET, Collaboration, Adriani, O., Asano, K., Bagliesi, M. G., Bigongiari, G., Binns, W. R., Bonechi, S., Bongi, M., Brogi, P., Buckley, J. H., Cannady, N., Castellini, G., Checchia, C., Cherry, M. L., Collazuol, G., Di, Felice V., Guzik, T. G., Hams, T., Ioka, K., Ishizaki, W., Israel, M. H., Javaid, A., Kataoka, R., Kato, C., Kawanaka, N., Kawakubo, Y., Krawczynski, H. S., Krizmanic, J. F., Lomtadze, T., Maestro, P., Marrocchesi, P. S., Messineo, A. M., Mitchell, J. W., Miyake, S., Moiseev, A. A., Mori, M., Mori, N., Motz, H. M., Munakata, K., de, Nolfo G. A., Ormes, J. F., Ozawa, Shunsuke, Pacini, L., Palma, F., Papini, P., Penacchioni, A. V., Rauch, B. F., Ricciarini, S. B., Sakai, K., Sakamoto, T., Sasaki, M., Shimizu, Yuki, Shiomi, A., Sparvoli, R., Spillantini, P., Stolzi, F., Takahashi, I., Takita, M., Tsunesada, Y., Vannuccini, E., Wefel, J. P., Yamaoka, K., Yanagita, S., Yoshida, A., Akaike, Yosui, Asaoka, Yoichi, Ebisawa, Ken, Fuke, Hideyuki, Hareyama, Makoto, Hasebe, Nobuyuki, Hibino, Kinya, Ichimura, Masakatsu, Kasahara, Katsuaki, Kataoka, Jun, Katayose, Yusaku, Kuramata, Shiyuuichi, Mizutani, Kouhei, Mori, Kunishiro, Murakami, Hiroyuki, Nakahira, Satoshi, Nishimura, Jun, Okuno, Shoji, Takayanagi, Masahiro, Tamura, Tadahisa, Tateyama, Nobuhito, Terasawa, Toshio, Tomida, Hiroshi, Torii, Shoji, Uchihori, Yukio, Ueno, Shiro, Yoshida, Kenji, Yuda, Toshinori

Publikováno v: Physical review letters
119 (2017): 181101-1–181101-6. doi:10.1103/PhysRevLett.119.181101
info:cnr-pdr/source/autori:Adriani O.; Akaike Y.; Asano K.; Asaoka Y.; Bagliesi M.G.; Bigongiari G.; Binns W.R.; Bonechi S.; Bongi M.; Brogi P.; Buckley J.H.; Cannady N.; Castellini G.; Checchia C.; Cherry M.L.; Collazuol G.; Di Felice V.; Ebisawa K.; Fuke H.; Guzik T.G.; Hams T.; Hareyama M.; Hasebe N.; Hibino K.; Ichimura M.; Ioka K.; Ishizaki W.; Israel M.H.; Javaid A.; Kasahara K.; Kataoka J.; Kataoka R.; Katayose Y.; Kato C.; Kawanaka N.; Kawakubo Y.; Krawczynski H.S.; Krizmanic J.F.; Kuramata S.; Lomtadze T.; Maestro P.; Marrocchesi P.S.; Messineo A.M.; Mitchell J.W.; Miyake S.; Mizutani K.; Moiseev A.A.; Mori K.; Mori M.; Mori N.; Motz H.M.; Munakata K.; Murakami H.; Nakahira S.; Nishimura J.; De Nolfo G.A.; Okuno S.; Ormes J.F.; Ozawa S.; Pacini L.; Palma F.; Papini P.; Penacchioni A.V.; Rauch B.F.; Ricciarini S.B.; Sakai K.; Sakamoto T.; Sasaki M.; Shimizu Y.; Shiomi A.; Sparvoli R.; Spillantini P.; Stolzi F.; Takahashi I.; Takayanagi M.; Takita M.; Tamura T.; Tateyama N.; Terasawa T.; Tomida H.; Torii S.; Tsunesada Y.; Uchihori Y.; Ueno S.; Vannuccini E.; Wefel J.P.; Yamaoka K.; Yanagita S.; Yoshida A.; Yoshida K.; Yuda T./titolo:Energy Spectrum of Cosmic-Ray Electron and Positron from 10 GeV to 3 TeV Observed with the Calorimetric Electron Telescope on the International Space Station/doi:10.1103%2FPhysRevLett.119.181101/rivista:Physical review letters (Print)/anno:2017/pagina_da:181101-1/pagina_a:181101-6/intervallo_pagine:181101-1–181101-6/volume:119

First results of a cosmic-ray electron + positron spectrum, from 10 GeV to 3 TeV, is presented based upon observations with the CALET instrument on the ISS starting in October, 2015. Nearly a half million electron + positron events are included in th

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9be600f35cf51ccadaf2cf4a020c8ceb
https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.119.181101

A future plan in observing ultra-heavy nuclei (Z=30-110) of cosmic rays with large-scale collector at the lunar base

Autor: Hasebe, Nobuyuki, Kodaira, Satoshi, Hareyama, Makoto, Yasuda, Nakahiro

Publikováno v: Radiation Measurements. 44(9-10):913-916

Lunar-based measurement of galactic cosmic ray (GCR) nuclei with a high precision is a challenging approach in cosmic ray research for the coming 20 years. This approach focuses to measure the elemental composition of Pt- and Pb-groups, actinide and

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::46622bdcdd2ec90280e4314755f1737b
https://repo.qst.go.jp/records/45717