TY - GEN
T1 - Performance of the CALET prototype
T2 - 32nd International Cosmic Ray Conference, ICRC 2011
AU - Karube, Mikihiko
AU - Torii, Shoji
AU - Kasahara, Katsuaki
AU - Ozawa, Shunsuke
AU - Akaike, Yosui
AU - Aiba, Toshihide
AU - Ueyama, Yoshitaka
AU - Nakamura, Masanori
AU - Yoshida, Keisuke
AU - Tamura, Tadahisa
AU - Okuno, Shoji
AU - Katayose, Yusaku
AU - Shimizu, Yuki
PY - 2011
Y1 - 2011
N2 - We are developing the CALET mission to observe high energy cosmic rays at the Japanese Experiment Module/Exposed Facility (JEM/EF) on the International Space Station. The instrument will be flown in 2013, and will be used for 5 years. The primary scientific purpose of CALET is to search for nearby cosmic ray sources and dark matter. We carried out an accelerator beam test with high energy particles with the CALET prototype at the CERN-SPS. The purpose of this test was to assess the detector performance as well as to study the accuracy of the Monte Carlo simulation method. The prototype detector consists of an imaging calorimeter with 256 scintillating fibers and a total absorption calorimeter consisting of 16 PWO logs. The longitudinal structure is similar with the CALET instrument. We used positron and proton beams in the energy region from 6 to 200 GeV, and from 30 to 150 GeV, respectively. Comparing the experimental data with the simulation results, we have measured the energy deposition in each component, the energy resolution, the lateral shower spread and the e/p separation capability.
AB - We are developing the CALET mission to observe high energy cosmic rays at the Japanese Experiment Module/Exposed Facility (JEM/EF) on the International Space Station. The instrument will be flown in 2013, and will be used for 5 years. The primary scientific purpose of CALET is to search for nearby cosmic ray sources and dark matter. We carried out an accelerator beam test with high energy particles with the CALET prototype at the CERN-SPS. The purpose of this test was to assess the detector performance as well as to study the accuracy of the Monte Carlo simulation method. The prototype detector consists of an imaging calorimeter with 256 scintillating fibers and a total absorption calorimeter consisting of 16 PWO logs. The longitudinal structure is similar with the CALET instrument. We used positron and proton beams in the energy region from 6 to 200 GeV, and from 30 to 150 GeV, respectively. Comparing the experimental data with the simulation results, we have measured the energy deposition in each component, the energy resolution, the lateral shower spread and the e/p separation capability.
KW - Beam test
KW - Calorimeter
KW - CERN-SPS
KW - Monte carlo simulation
UR - http://www.scopus.com/inward/record.url?scp=84899517706&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84899517706&partnerID=8YFLogxK
U2 - 10.7529/ICRC2011/V06/0835
DO - 10.7529/ICRC2011/V06/0835
M3 - Conference contribution
AN - SCOPUS:84899517706
VL - 6
SP - 383
EP - 386
BT - Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011
PB - Institute of High Energy Physics
Y2 - 11 August 2011 through 18 August 2011
ER -