The cosmic ray energetics and mass for the international space station (ISS-CREAM) instrument

被引：2

作者：

Yoon, Y. S. ^{[1
,2
,10
]}

Amare, Y. ^{[1
]}

Angelaszek, D. ^{[1
,2
]}

Anthony, N. ^{[2
]}

Cheryian, K. ^{[2
]}

Choi, G. H. ^{[3
,17
]}

Copley, M. ^{[1
]}

Coutu, S. ^{[4
]}

Derome, L. ^{[5
]}

Eraud, L. ^{[5
]}

Hagenau, L. ^{[2
]}

Han, J. H. ^{[1
]}

Huh, H. G. ^{[1
]}

Hwang, Y. S. ^{[6
,11
]}

Hyun, H. J. ^{[6
,12
]}

Im, S. ^{[4
]}

Jeon, H. B. ^{[6
,13
]}

Jeon, J. A. ^{[3
,14
]}

Jeong, S. ^{[3
]}

Kang, S. C. ^{[6
]}

Kim, H. J. ^{[6
]}

Kim, K. C. ^{[1
]}

Kim, M. H. ^{[1
]}

Lee, H. Y. ^{[4
,14
]}

Lee, M. H. ^{[1
,14
]}

Liang, J. ^{[2
]}

Lu, L. ^{[2
]}

Lutz, L. ^{[1
]}

Menchaca-Rocha, A. ^{[8
]}

Mitchell, J. W. ^{[7
]}

Mognet, S. I. ^{[2
]}

Morton, S. ^{[2
]}

Nester, M.

Nutter, S. ^{[9
]}

Park, H.

Park, I. H.

Park, J. M. ^{[6
,15
]}

Picot-Clemente, N. ^{[1
]}

Seo, E. S. ^{[1
,2
]}

Smith, J. R. ^{[1
]}

Walpole, P. ^{[1
]}

Weinmann, R. P. ^{[1
]}

Wu, J. ^{[1
]}

Zhang, H. G. ^{[1
,16
]}

机构：

[1] Univ Maryland, Inst Phys Sci & Tech, College Pk, MD 20742 USA

[2] Univ Maryland, Dept Phys, College Pk, MD 20742 USA

[3] Sungkyunkwan Univ, Dept Phys, Suwon 16419, South Korea

[4] Penn State Univ, Dept Phys, University Pk, PA 16802 USA

[5] Univ Grenoble Alpes, CNRS, IN2P3, LPSC, LPSC-IN2P3, F-38000 Grenoble, France

[6] Kyungpook Natl Univ, Dept Phys, Daegu 41566, South Korea

[7] NASA Goddard Space Flight Ctr, Astroparticle Phys Lab, Greenbelt, MD 20771 USA

[8] Univ Nacl Autonoma Mexico, Inst Fis, Ciudad Univ, Mexico City 04510, Mexico

[9] Northern Kentucky Univ, Dept Phys & Geol, Highland Hts, KY 41099 USA

[10] Korea Res Inst Stand & Sci, Daejeon 34113, South Korea

[11] Korea Atom Energy Res Inst KOMAC, Daejeon 38180, Gyeongbuk, South Korea

[12] Pohang Accelerator Lab, Pohang 37673, Gyeongbuk, South Korea

[13] Univ Chicago, Chicago, IL 60637 USA

[14] Inst for Basic Sci Korea, Daejeon 34126, South Korea

[15] Korea Atom Energy Res Inst, Inst Adv Rad Tech, Daejeon 56212, Jeonbuk, South Korea

[16] Beijing Jiao Tong Univ, Beijing 100044, Peoples R China

[17] Korea Aerosp Res Inst, Daejeon 34133, South Korea

来源：

ASTROPARTICLE PHYSICS | 2024年 / 158卷

基金：

新加坡国家研究基金会;

关键词：

Cosmic -ray instrument; Direct measurements; International space station; TeV; Elemental spectra measurements; BOTTOM COUNTING DETECTORS; SILICON CHARGE DETECTOR; PERFORMANCE; NUCLEI; FLIGHT; TOP;

D O I：

10.1016/j.astropartphys.2024.102947

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 similar to 10(12) to similar to 10(15) 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.

引用

页数：13

共 39 条

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