Performance of the SciCR as a solar neutron detector

机译：SciCR作为太阳中子探测器的性能

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The SciCR, SciBar for the Cosmic Ray Observation, is a new multi-purpose cosmic ray experiment. The main aim of the SciCR is the detection of solar neutrons, and it will operate at Mt. Sierra Negra in Mexico, at 4.600m above sea level. The detector is made of 15,000 plastic scintillator bars. The dimension of each bar is 2.5cm ×1.3cm × 3m. We made a small prototype experiment called as mini-SciCR, using the same scintillator bars, with smaller length (20cm). Otie of the purposes of the mini-SciCR is to test the hardware of the experiment at Mt. Sierra Negra before the installation of the SciCR. The other purpose is to measure the cosmic ray baclcground. We will present the result of the mini-SciCR experiment, and the detection efficiency of SciCR for solar neutrons obtained by a Monte Carlo simulation taking into account the mini-SciCR results.

机译：SciCR，即用于宇宙射线观测的SciBar，是一种新的多功能宇宙射线实验。 SciCR的主要目的是探测太阳中子，它将在Mt. Mt.上运行。墨西哥内格拉山脉，海拔4.600m。检测器由15,000个塑料闪烁棒制成。每个条的尺寸为2.5cm×1.3cm×3m。我们使用相同的闪烁棒（长度较短（20厘米））进行了一个小型实验，称为mini-SciCR。 mini-SciCR的主要目的是在Mt.测试硬件的实验。 SciCR安装之前的Sierra Negra。另一个目的是测量宇宙射线bacground。我们将介绍mini-SciCR实验的结果，并考虑到mini-SciCR结果，通过蒙特卡洛模拟获得的太阳中子对SciCR的检测效率。

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来源
《International Cosmic Ray Conference》|2011年|1-4|共4页
会议地点 Beijing(CN)
作者
Y. Nagai; M. Kozai; M. Tsurusashi; Y. Nakano; S. Shibata; H. Takamaru; H. Kojima; H. Tsuchiya; K. Watanabe; T. Koi; J. F. Valdes-Galicia; Y. Matsubara; A. Hurutado; O. Musalem; E. Ortiz; L. X. Gonzalez; Y. Itow; T. Sako; D. Lopez; G. Mitsuka; K. Munakata; C. Kato; S.Yasue;
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作者单位

Solar-Terrestrial Environment Laboratory Nagoya University Furo-cho Chikusa-ku Nagoya 464-8601 Japan;

Department of Physics Shinshu University Asahi Matsumoto 390-8621 Japan;

College of Engineering Chubu University Kasugai 487-8501 Japan;

Faculty of Engineering Aichi Institute of Technology Toyota 470-0392 Japan;

High-energy Astrophysics Laboratory Riken Hirosawa Wako 351-0198 Japan;

Institute of Space and Astronautical Science Japan Aerospace Exploration Agency Yoshinodai chuo-ku Saganuhara 252-5210;

SLAC National Accelerator Laboratory MenloPark CA 94025-7015 USA;

Instituto de Geofisica Universidad Nacional Autonoma de Mexico Ciudad Universitaria Coyoacan DF 04510 Mexico;

Solar-Terrestrial Environment Laboratory Nagoya University Furo-cho Chikusa-ku Nagoya 464-8601 Japan;

Institute de Astrofisica Optica y Electronica Tonantzintla Pitebla C.P. 72840 Puebla Mexico;

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solar neutron; sensitive cosmic ray detector; SciCR;

机译：太阳中子灵敏的宇宙射线探测器；科学文摘;

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2. Physical-chemical characterization of a GEM side-on ~(10)B-based thermal neutron detector and analysis of its neutron diffraction performances [J] . A. Santoni, G. Celentano, G. Claps, Nuclear Instruments & Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment . 2018,第OCTa21期

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3. Detection of high-energy solar neutrons and protons by ground level detectors on April 15, 2001 [J] . Muraki Y, Matsubara Y, Masuda S, Astroparticle physics . 2008,第4期

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4. Performance of the SciCR as a solar neutron detector [C] . Y. Nagai, M. Kozai, M. Tsurusashi, International Cosmic Ray Conference . 2011

机译：SCICR作为太阳中子探测器的性能
5. Fusion and Solar Plasmas: Synergistic Effects of Neutrons and Plasma on Materials in Fusion Reactors & Relaxation of Merging Magnetic Flux Ropes In Fusion and Solar Plasmas [D] . Hussain, Asad S. 2018

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6. Commissioning of the NPDGamma Detector Array: Counting Statistics in Current Mode Operation and Parity Violation in the Capture of Cold Neutrons on B4C and 27Al [O] . M. T. Gericke, J. D. Bowman, R. D. Carlini, 2005

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7. Performance of the SciBar cosmic ray telescope (SciCRT) toward the detection of high-energy solar neutrons in solar cycle 24 [O] . Yoshinori Sasai, Yuya Nagai, Yoshitaka Itow, 2014

机译：SciBar宇宙射线望远镜（SciCRT）在太阳周期24中检测高能太阳中子的性能
8. Development of the OSO-6 High-Energy Neutron Detector and Correlation of Measured Solar Neutron Fluxes to Solar Flares [R] . Frederick Young 1974

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Performance of the SciCR as a solar neutron detector

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