共查询到19条相似文献,搜索用时 156 毫秒
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带电粒子在材料中的剂量深度分布计算 总被引:4,自引:3,他引:1
航天器在轨道运行期间,会受到各种带电粒子的作用,其能量沉积在表面材料中,对表面材料的性能有较大的损伤。文章介绍了剂量深度计算程序,利用SRIM及ITS软件的计算结果,计算出了带电粒子在材料中的剂量深度分布,并对空间轨道实际环境下材料中的剂量深度分布进行了计算。利用这一程序,在“东四”热控涂层试验中进行了剂量深度分布拟合,计算了多种能量电子拟合试验下荆量深度分布与空间实际环境的比较,得出了相关的试验参数。 相似文献
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原子氧对低地球轨道(LEO)卫星表面的剥蚀已为众多的飞行试验所证实,它对热控涂层、光学表面的损伤是明显的.随着LEO卫星性能的提高和工作寿命的增长,应把原子氧对材料的剥蚀试验作为LEO卫星表面用材料的筛选试验,推荐原子氧对材料的剥蚀试验条件为 1.0×1020~3.0×1020个/cm2.试验设备应配有紫外,二者协合能更好地模拟轨道上的效应.开展LEO卫星上的搭载飞行试验,确定原子氧环境对材料的影响,逐步建立起原子氧效应数据库,对加速载人航天和空间站技术的发展是必要的. 相似文献
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文章着眼于提高地球同步轨道(GEO)空间地磁亚暴带电效应模拟的真实度,对多能量电子模拟空间地磁亚暴带电的方法进行分析评估。首先采用单一能量电子束的地面试验对SENSIT工程软件进行了校准;然后参考地磁亚暴环境能谱,用该软件对Kapton样品在单一电子束、双电子束、全能谱电子辐照下的充放电特性进行了计算预示。研究表明:表面充电速率受控于电流密度;在12.5keV/32.5keV电子束组合时其效应模拟的结果最有代表性;在双电子束模拟中,较高能量电子源起关键作用。 相似文献
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氮化镓(GaN)基异质结材料以其宽禁带、耐高温、高击穿电压以及优异的抗辐射性能成为航天领域半导体材料的研究和应用热点。而基于GaN材料的AlGaN/GaN高电子迁移率晶体管(HEMT)因其制备过程带来的缺陷和损伤,性能将受到空间辐射的严峻挑战。文章对空间辐射环境下AlGaN/GaN HEMT的辐射机理和效应进行梳理;针对低中地球轨道以质子为主的辐射环境,对不同能量和注量的质子辐照对AlGaN/GaN HEMT的效应进行系统分析。鉴于从压电极化角度分析AlGaN/GaN HEMT的质子辐射效应存在欠缺,且不同能量和注量的质子辐照对器件的影响不同,提出后续应开展AlGaN/GaN HEMT辐射损伤机制、不同轨道辐射环境模拟以及质子辐照对AlGaN/GaN HEMT宏观特性影响研究。 相似文献
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The aim of this paper is to present the time profile of cosmic radiation exposure obtained by the Radiation Risk Radiometer-Dosimeter during the EXPOSE-E mission in the European Technology Exposure Facility on the International Space Station's Columbus module. Another aim is to make the obtained results available to other EXPOSE-E teams for use in their data analysis. Radiation Risk Radiometer-Dosimeter is a low-mass and small-dimension automatic device that measures solar radiation in four channels and cosmic ionizing radiation as well. The main results of the present study include the following: (1) three different radiation sources were detected and quantified-galactic cosmic rays (GCR), energetic protons from the South Atlantic Anomaly (SAA) region of the inner radiation belt, and energetic electrons from the outer radiation belt (ORB); (2) the highest daily averaged absorbed dose rate of 426 μGy d(-1) came from SAA protons; (3) GCR delivered a much smaller daily absorbed dose rate of 91.1 μGy d(-1), and the ORB source delivered only 8.6 μGy d(-1). The analysis of the UV and temperature data is a subject of another article (Schuster et al., 2012 ). 相似文献
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Paulino-Lima IG Janot-Pacheco E Galante D Cockell C Olsson-Francis K Brucato JR Baratta GA Strazzulla G Merrigan T McCullough R Mason N Lage C 《Astrobiology》2011,11(9):875-882
In this experimental study, cells of the radiation-resistant bacterium Deinococcus radiodurans were exposed to several different sources of radiation chosen to replicate the charged particles found in the solar wind. Naked cells or cells mixed with dust grains (basalt or sandstone) differing in elemental composition were exposed to electrons, protons, and ions to determine the probability of cell survival after irradiation. Doses necessary to reduce the viability of cell population to 10% (LD(10)) were determined under different experimental conditions. The results of this study indicate that low-energy particle radiation (2-4?keV), typically present in the slow component of the solar wind, had no effect on dehydrated cells, even if exposed at fluences only reached in more than 1000 years at Sun-Earth distance (1 AU). Higher-energy ions (200?keV) found in solar flares would inactivate 90% of exposed cells after several events in less than 1 year at 1 AU. When mixed with dust grains, LD(10) increases about 10-fold. These results show that, compared to the highly deleterious effects of UV radiation, solar wind charged particles are relatively benign, and organisms protected under grains from UV radiation would also be protected from the charged particles considered in this study. 相似文献
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A.N. Denisov N.V. Kuznetsov R.A. Nymmik M.I. Panasyuk N.M. Sobolevsky 《Acta Astronautica》2011,68(9-10):1440-1447
In connection with projects on a manned base on the Moon, the assessment of radiation risk to staff of the base owing to galactic (GCR) and solar (SEP) cosmic radiation becomes very relevant. The paper describes the methodology for assessing the radiation environment on the lunar surface and in the depths of lunar soil taking into account the primary and secondary radiation caused by protons and nuclei of GCR and SEP. Calculated fluencies of particles are used to estimate the average annual absorbed and equivalent local doses in tissue. Contribution to the dose of secondary neutrons at depths of lunar soil exceeds the contribution of protons. Contribution to the dose of secondary particles generated by GCR nuclei should be taken into account. 相似文献
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M. I. Panasyuk M. V. Podzolko A. S. Kovtyukh I. A. Brilkov N. A. Vlasova V. V. Kalegaev V. I. Osedlo V. I. Tulupov I. V. Yashin 《Cosmic Research》2017,55(2):79-87
The Earth’s radiation belts discovered at the end of the 1950s have great scientific and practical interest. Their main characteristics in magnetically quiet periods are well known. However, the dynamics of the Earth’s radiation belts during magnetic storms and substorms, particularly the dynamics of relativistic electrons of the outer belt, when Earth’s radiation belt particle fluxes undergo significant time variations, is studied insufficiently. At present, principally new experiments have been performed and planned with the intention to better study the dynamics of the Earth’s radiation belts and to operationally control the space-energy distributions of the Earth’s radiation belt particle fluxes. In this paper, for spacecraft designed to measure the fluxes of electrons and protons of the Earth’s radiation belts at altitudes of 0.5–10000 km, the optimal versions for detector orientation and orbital parameters have been considered and selected. 相似文献
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A. N. Denisov N. V. Kuznetsov R. A. Nymmik M. I. Panasyuk N. M. Sobolevskii 《Cosmic Research》2010,48(6):509-516
In connection with projects of manned bases on the Moon it becomes topical to estimate radiation danger for their inhabitants.
In this paper we describe a method of evaluation of the radiation environment on the lunar surface produced by galactic and
solar cosmic rays. The roles of both primary and secondary radiations generated in the depth of the lunar soil under the action
of high-energy protons and nuclei are taken into account. Calculated fluxes of particles are used in order to estimate annual
averaged absorbed and equivalent local dose rates in tissues. It is established that in the lunar rock the contribution of
secondary neutrons to the dose rate exceeds that of protons. The contribution of the secondary particles generated by nuclei
of galactic cosmic rays to the dose rate is estimated. 相似文献
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Calorimeters are used in cosmic ray studies for a variety of purposes, such as measurements of particle energy, separation
of electrons and hadrons, formation of triggers (signals for activation of instruments), and so on. In this review we consider
the methods of energy reconstruct of protons and electrons (for particles with energies exceeding 10 GeV) in calorimeters
of various types that are used in astrophysical experiments of cosmic ray studies carried out with balloons and satellites. 相似文献
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Kuznetsov N. V. Nymmik R. A. Panasyuk M. I. Sosnovets E. N. Teltsov M. V. 《Cosmic Research》2004,42(3):203-209
We consider cases of simultaneous detection of the absorbed doses produced by proton fluxes of powerful solar events onboard the Mir and ISS orbital stations and the Ekspress A3 geosynchronous satellite. Experimental data are analyzed using a software package that takes into account the energy spectra of protons at the Earth's orbit depending on the time of event evolution, as well as their penetration to near-earth orbits and through the protective shields of spacecraft. Based on a comparison of the experimental data of dosimeters with the calculation of absorbed doses under the action of solar proton events, we developed a method of estimating the effective thickness of the shielding of dosimeters and made some estimates. A possibility is considered for predicting the radiation hazard onboard orbital stations upon the appearance of solar proton events using dosimeter data from a geosynchronous orbit. 相似文献