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DOSIS & DOSIS 3D: radiation measurements with the DOSTEL instruments onboard the Columbus Laboratory of the ISS in the years 2009–2016

机译:DOSIS和DOSIS 3D:2009-2016年间,使用ISSTEL仪器在国际空间站哥伦布实验室上进行辐射测量

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The natural radiation environment in Low Earth Orbit (LEO) differs significantly in composition and energy from that found on Earth. The space radiation field consists of high energetic protons and heavier ions from Galactic Cosmic Radiation (GCR), as well as of protons and electrons trapped in the Earth’s radiation belts (Van Allen belts). Protons and some heavier particles ejected in occasional Solar Particle Events (SPEs) might in addition contribute to the radiation exposure in LEO. All sources of radiation are modulated by the solar cycle. During solar maximum conditions SPEs occur more frequently with higher particle intensities. Since the radiation exposure in LEO exceeds exposure limits for radiation workers on Earth, the radiation exposure in space has been recognized as a main health concern for humans in space missions from the beginning of the space age on. Monitoring of the radiation environment is therefore an inevitable task in human spaceflight. Since mission profiles are always different and each spacecraft provides different shielding distributions, modifying the radiation environment measurements needs to be done for each mission. The experiments “Dose Distribution within the ISS (DOSIS)” (2009–2011) and “Dose Distribution within the ISS 3D (DOSIS 3D)” (2012–onwards) onboard the Columbus Laboratory of the International Space Station (ISS) use a detector suite consisting of two silicon detector telescopes (DOSimetry TELescope?=?DOSTEL) and passive radiation detector packages (PDP) and are designed for the determination of the temporal and spatial variation of the radiation environment. With the DOSTEL instruments’ changes of the radiation composition and the related exposure levels in dependence of the solar cycle, the altitude of the ISS and the influence of attitude changes of the ISS during Space Shuttle dockings inside the Columbus Laboratory have been monitored. The absorbed doses measured at the end of May 2016 reached up to 286?μGy/day with dose equivalent values of 647?μSv/day.
机译:低地球轨道(LEO)中的自然辐射环境在成分和能量上与地球上发现的自然环境不同。太空辐射场包括高能质子和来自银河宇宙辐射(GCR)的重离子,以及俘获在地球辐射带(范艾伦带)中的质子和电子。偶尔发生的太阳粒子事件(SPE)中喷出的质子和一些较重的粒子可能还有助于LEO中的辐射暴露。所有辐射源均受太阳周期的调制。在最高日照条件下,固相萃取会以较高的颗粒强度发生得更频繁。由于LEO中的辐射暴露超过了地球上辐射工作者的暴露极限,因此从太空时代开始,在太空飞行中,人们就已经认识到太空中的辐射暴露是人类主要的健康问题。因此,辐射环境的监测是人类航天飞行中不可避免的任务。由于任务概况总是不同的,并且每个航天器提供不同的屏蔽分布,因此需要针对每个任务修改辐射环境的测量值。在国际空间站(ISS)哥伦布实验室上进行的“国际空间站(DOSIS)剂量分布”(2009-2011年)和“国际空间站3D剂量分布(DOSIS 3D)”(2012年及以后)实验使用了探测器该套件由两个硅探测器望远镜(DOSimetry TELescope?=?DOSTEL)和无源辐射探测器套件(PDP)组成,旨在确定辐射环境的时空变化。利用DOSTEL仪器随着太阳周期的变化而改变了辐射成分和相关的暴露水平,在哥伦布实验室内部的航天飞机对接期间,国际空间站的高度和国际空间站的姿态变化的影响得到了监测。 2016年5月底测得的吸收剂量高达286?μGy/天,剂量当量值为647?μSv/天。

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