高能离子辐照下薄膜界面化学结合增强的模型

近年来高能离子辐照引起的薄膜附着力增强现象及其应用受到了广泛的重视。由于高能离子一固体相互作用的复杂性,目前对附着力增强的物理机制的认识还不清楚。文章基于高能离子辐照引起界面原子化学结合键增强的思想,建立了薄膜附着力增强的理论模型,并由此得到辐照离子阈剂量与离子能量损失(电子阻止能力)及其界面原子结合键能的分析表达式,计算结果与实验结果很好吻合。理论分析表达式说明,膜附着力增强的阈剂量受界面原子结构、元素种类、电子阻止能力及其形成固体径迹所损失的能量等多种因素有关。     

耐辐照光纤的瞬态辐照实验及峰值感生损耗的测定

应用相对论强流电子脉冲加速器作辐射源,建立了一套实验系统,对耐辐照光纤进行了瞬态大剂量X射线辐照实验与研究,并同当今国际上先进的同种类光纤进行了对比,获得了瞬态峰值感生损耗等很有价值的实验结果。     

ASAP: A systematic approach to plasma spectral synthesis

ASAP (Analysis System for Astrophysical Plasmas), developed at the Osservatorio Astronomico di Palermo, is a package of procedures based on IDL. It is aimed at the detailed presentation of theoretical models of astrophysical plasmas and the accurate comparison with observational data, up to fittings of specific observations. It is also useful for the prediction of specific observations, and for the simulation of the expected performances of forthcoming instruments, for instance those on board SOHO.     

原子氧与真空紫外线协同效应对有机涂层的降解作用

为研究真空紫外与原子氧的协同作用,进行了环氧树脂和有机硅树脂的原子氧/真空紫外交互的地面模拟实验,结果表明:在交互作用中,对有机涂层破坏的主导因素是原子氧,真空紫外线起到协同作用,在切断有机高分子材料化学键的同时,为原子氧提供了反应基,加速了原子氧的反应速率.对比真空紫外辐照和原子氧/真空紫外交互实验结果分析中可以发现,有机硅树脂是较好的耐真空紫外辐射和原子氧侵蚀的有机涂层材料.     

The status and future of EUV astronomy

The Extreme Ultraviolet wavelength range was one of the final windows to be opened up to astronomy. Nevertheless, it provides very important diagnostic tools for a range of astronomical objects, although the opacity of the interstellar medium restricts the majority of observations to sources in our own galaxy. This review gives a historical overview of EUV astronomy, describes current instrumental capabilities and examines the prospects for future facilities on small and medium-class satellite platforms.     

Lunar exosphere influence on lunar-based near-ultraviolet astronomical observations

The potential effect of the lunar exosphere on the near-ultraviolet sky background emission is predicted for Lunar-based Ultraviolet Telescope (LUT: a funded Chinese scientific payload for the Chang’e-III mission). Using the upper limit on the OH concentration inferred from the recent MIP CHACE results, our calculations show that the sky brightness due to the illuminated exosphere is <8.7 photons⁻¹ cm⁻² arcsec⁻² within the wavelength range 245–340 nm. By evaluating the signal-to-noise ratios of observations of an AB = 13 mag point source at a series of sky background levels, our analysis indicates that the detection performance of LUT can be moderately degraded by the lunar exosphere emission in most cases. An AB = 13 mag point source can still be detected by the telescope at a signal-to-noise ratio more than 8 when the OH concentration is less than 2 × 10⁸ molecules cm⁻³. However, the effect on the performance is considerable when the exosphere is as dense as suggested by CHACE.     

No significant level of inheritable interchromosomal aberrations in the progeny of bystander primary human fibroblasts after alpha particle irradiation

A major concern for bystander effects is the probability that normal healthy cells adjacent to the irradiated cells become genomically unstable and undergo further carcinogenesis after therapeutic irradiation or space mission where astronauts are exposed to low dose of heavy ions. Genomic instability is a hallmark of cancer cells. In the present study, two irradiation protocols were performed in order to ensure pure populations of bystander cells and the genomic instability in their progeny were investigated. After irradiation, chromosomal aberrations of cells were analyzed at designated time points using G₂ phase premature chromosome condensation (G₂-PCC) coupled with Giemsa staining and with multiplex fluorescent in situ hybridization (mFISH). Our Giemsa staining assay demonstrated that elevated yields of chromatid breaks were induced in the progeny of pure bystander primary fibroblasts up to 20 days after irradiation. mFISH assay showed no significant level of inheritable interchromosomal aberrations were induced in the progeny of the bystander cell groups, while the fractions of gross aberrations (chromatid breaks or chromosomal breaks) significantly increased in some bystander cell groups. These results suggest that genomic instability occurred in the progeny of the irradiation associated bystander normal fibroblasts exclude the inheritable interchromosomal aberration.     

航天材料紫外辐射效应地面模拟试验方法

空间紫外辐射环境可造成航天器材料的光学性能、电学性能或力学性能退化甚至失效。在地面模拟试验过程中较难真实模拟空间紫外辐射环境,因此,通常采用基于效应等效原理的加速模拟试验方法。文章首先对国内外紫外辐射效应试验方法和标准现状进行梳理,进而从紫外曝辐量的计算方法、紫外波长的选择、模拟光源选用、温度选择与控制以及总曝辐量和加速因子的选择等角度对紫外辐射效应地面模拟试验方法进行分析研究,并给出应进一步开展工作的建议。     

MOS电容器单粒子介质击穿导致GaN功率放大器失效分析

为验证一款GaN功率放大器抗空间辐射效应能力,对其进行了重离子单粒子效应试验研究。被试样品是由GaN HEMT、MOS电容器和电感器等组成的混合电路。试验源为加速器产生的锗离子（Ge+13,能量205 MeV),线性能量传输（LET）值为37.4 MeV·cm2/mg。试验结果是：GaN HEMT性能未出现变化;MOS电容器发生了介质击穿失效,造成功率放大器功能失效。经验公式计算的单粒子介质击穿电压,与重离子试验结果基本吻合,得出MOS电容器单粒子介质击穿导致GaN功率放大器失效。研究表明,混合电路中无源的MOS电容器也会发生单粒子介质击穿失效,应用于空间环境时应进行单粒子效应评估。     

APS星敏感器太阳照射影响分析及试验验证

针对APS星敏感器在轨过程中太阳照射问题进行了研究,分析了太阳照射对星敏感器功能和性能的影响,设计了太阳照射相关的试验及验证方案,最后给出了相关试验过程和试验验证结果,明确了分析及试验结论.通过分析和试验结果表明:紫外辐照试验对光学系统透过率无明显影响,且影响在APS星敏感器灵敏度余量范围内;在轨太阳照射对APS星敏感器探测器及整机的功能和性能无影响.相关分析和试验数据可作为星敏感器后续改进设计的依据和参考.