国际空间站宇宙射线能量和质量(ISS-CREAM)仪器

IF 4.2 3区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Y.S. Yoon , Y. Amare , D. Angelaszek , N. Anthony , K. Cheryian , G.H. Choi , M. Copley , S. Coutu , L. Derome , L. Eraud , L. Hagenau , J.H. Han , H.G. Huh , Y.S. Hwang , H.J. Hyun , S. Im , H.B. Jeon , J.A. Jeon , S. Jeong , S.C. Kang , H.G. Zhang
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引用次数: 0

摘要

国际空间站-CREAM 仪器是宇宙射线能量和质量(CREAM)实验的改进版,该实验曾多次在南极洲上空用气球飞行,后来安装在国际空间站上。其主要目标是测量 Z = 1 到 Z = 26 的电荷范围内,能量范围在 ∼ 1012 到 ∼ 1015 eV 之间的单个宇宙射线元素的能谱。该仪器包括一个钨/闪烁体量热计和一个像素化硅电荷探测器作为主探测器,用于确定宇宙射线的能量和电荷。此外,它还包括顶部和底部闪烁体计数探测器和一个硼化闪烁体探测器,用于区分电子和强子,以进行多太伏电子测量。ISS-CREAM仪器于2017年8月安装在国际空间站上,运行至2019年2月。本文概述了该仪器,重点介绍了其探测器、触发系统、通用电子设备和电源系统。本文重点介绍了为优化国际空间站运行性能而对这些组件进行的修改。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The cosmic ray energetics and mass for the international space station (ISS-CREAM) instrument

The ISS-CREAM instrument is the modified version of the Cosmic Ray Energetics And Mass (CREAM) experiment, which was flown on balloons multiple times over Antarctica and later installed on the International Space Station (ISS). Its primary objective is to measure the energy spectra of individual cosmic-ray elements for the charge range of Z = 1 to Z = 26, in the energy range of ∼ 1012 to ∼ 1015 eV. The instrument comprises a tungsten/scintillator calorimeter and a pixelated silicon charge detector as primary detectors to determine the energy and charge of cosmic rays. Additionally, it includes top and bottom scintillator counting detectors and a boronated scintillator detector to differentiate between electrons and hadrons for multi-TeV electron measurements. The ISS-CREAM instrument was installed on the ISS in August 2017 and operated until February 2019. This paper provides an overview of the instrument, focusing on its detectors, trigger systems, common electronics, and power systems. The paper highlights the modifications made to these components to optimize their performance for ISS operations.

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来源期刊
Astroparticle Physics
Astroparticle Physics 地学天文-天文与天体物理
CiteScore
8.00
自引率
2.90%
发文量
41
审稿时长
79 days
期刊介绍: Astroparticle Physics publishes experimental and theoretical research papers in the interacting fields of Cosmic Ray Physics, Astronomy and Astrophysics, Cosmology and Particle Physics focusing on new developments in the following areas: High-energy cosmic-ray physics and astrophysics; Particle cosmology; Particle astrophysics; Related astrophysics: supernova, AGN, cosmic abundances, dark matter etc.; Gravitational waves; High-energy, VHE and UHE gamma-ray astronomy; High- and low-energy neutrino astronomy; Instrumentation and detector developments related to the above-mentioned fields.
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