国际空间站辐射评估探测器的结果:第一部分,带电粒子探测器

IF 4.6 Q2 MATERIALS SCIENCE, BIOMATERIALS ACS Applied Bio Materials Pub Date : 2023-11-01 DOI:10.1016/j.lssr.2023.01.003
C. Zeitlin , A.J. Castro , K.B. Beard , M. Abdelmelek , B.M. Hayes , A.S. Johnson , N. Stoffle , R.R. Rios
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引用次数: 5

摘要

我们报告了2016年2月至2022年2月期间,使用辐射评估探测器(ISS-RAD)对国际空间站(ISS)高能粒子辐射环境进行的前六年测量的结果。第一个RAD是为火星科学实验室火星车MSL设计和建造的,也被称为“好奇号”;它自2012年以来一直在火星上运行,在这里被称为MSL-RAD。ISS-RAD结合了两个传感器头,一个几乎与单个MSL-RAD传感器头相同,另一个对快中子的灵敏度大大提高。这两个传感器头分别被称为带电粒子探测器(CPD)和快中子探测器(FND)。尽管名称如此,CPD也能够测量高能中子和γ射线,MSL-RAD也是如此。ISS-RAD于2015年12月飞往国际空间站,并于2016年2月部署,最初部署在美国实验室模块中。从2017年1月到2020年5月,RAD被用作测量仪器,当时该仪器被放置在美国实验室,并设置为天顶指向方向。国际空间站上的高能粒子环境很复杂,由于轨道相对于赤道的倾角为51.6∘,在这段时间内的高度在400–440公里之间,因此在短时间内变化很大。国际空间站在地磁场中持续移动,地磁场的强度随纬度、经度和高度而变化。轨道每天经过南大西洋异常(SAA)几次,磁捕获的质子和电子在那里产生观测通量和吸收剂量率的大幅度但短暂的增加。国际空间站内部的环境受到太阳周期、高度和局部屏蔽的影响,不同的国际空间站模块之间的屏蔽不同。我们报告了国际空间站中不同位置的带电粒子吸收剂量和剂量当量率的结果。在随附的论文中,我们报道了ISS-RAD快中子探测器获得的中子剂量当量率的类似结果。
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Results from the Radiation Assessment Detector on the International Space Station: Part 1, the Charged Particle Detector

We report the results of the first six years of measurements of the energetic particle radiation environment on the International Space Station (ISS) with the Radiation Assessment Detector (ISS-RAD), spanning the period from February 2016 to February 2022. The first RAD was designed and built for MSL, the Mars Science Laboratory rover, also known as Curiosity; it has been operating on Mars since 2012 and is referred to here as MSL-RAD. ISS-RAD combines two sensor heads, one nearly identical to the single MSL-RAD sensor head, the other with greatly enhanced sensitivity to fast neutrons. These two sensor heads are referred to as the Charged Particle Detector (CPD) and Fast Neutron Detector (FND), respectively. Despite its name, the CPD is also capable of measuring high-energy neutrons and γ-rays, as is MSL-RAD. ISS-RAD was flown to the ISS in December 2015 and was deployed in February 2016, initially in the USLab module. RAD was used as a survey instrument from January 2017 through May 2020, when the instrument was positioned in the USLab and set to a zenith-pointing orientation. The energetic particle environment on the ISS is complex and varies on short time scales owing to the orbit, which has a 51.6 inclination with respect to the equator and has had an altitude in the 400–440 km range in this time period. The ISS moves continuously through the geomagnetic field, the strength of which varies with latitude, longitude, and altitude. The orbit passes through the South Atlantic Anomaly (SAA) several times a day, where magnetically trapped protons and electrons produce large but transient increases in observed fluxes and absorbed dose rates. The environment inside the ISS is affected by the solar cycle, altitude, and the local shielding, which varies between different ISS modules. We report results for charged particle absorbed dose and dose equivalent rates in various positions in the ISS. In an accompanying paper, we report similar results for neutron dose equivalent rates obtained with the ISS-RAD Fast Neutron Detector.

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来源期刊
ACS Applied Bio Materials
ACS Applied Bio Materials Chemistry-Chemistry (all)
CiteScore
9.40
自引率
2.10%
发文量
464
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