Dust Acoustic Wave in Dusty Plasmas With Streaming Ions Under Ultraviolet Irradiation

The reductive perturbation method is applied to investigate the dust acoustic soliton in dusty plasmas with streaming ions under ultraviolet irradiation theoretically and numerically. The self-consistent dust charge variation is taken into account. It is shown that the ultraviolet irradiation can significantly lower the magnitude of the dust negative charge, and ion streaming velocity firstly raise the magnitude of the dust negative charge and then lower it. With the growth of (Ultraviolet) UV photo flux or ion streaming velocity, the phase velocity and width of the solitary waves decrease, whereas its amplitude increases.      

AVS-F observations of γ-ray emission during January 20, 2005 solar flare up to 140 MeV

The solar flare of January 20, 2005 (X7.1, 06:36–07:26 UT, maximum at 07:01 UT by the GOES soft X-ray data) was the most powerful one in January 2005 series. The AVS-F apparatus onboard CORONAS-F registered γ-emission during soft X-ray rising phase of this flare in two energy ranges of 0.1–20 MeV and 2–140 MeV. The highest γ-ray energy registered during this flare was ∼140 MeV. Six spectral features were registered in energy spectrum of this solar flare: annihilation + αα (0.4–0.6 MeV), ²⁴Mg + ²⁰Ne + ²⁸Si + neutron capture (1.7–2.3 MeV), ²¹Ne + ²²Ne + ¹⁶O + ¹²С (3.2–5.0 MeV), ¹⁶O (5.3–6.9 MeV), one from neutral pions decay (25–110 MeV) and one in energy band 15–21 MeV. Four of them contain typical for solar flares lines – annihilation, nuclear de-excitation and neutron capture at ¹H. Spectral feature caused by neutral pions decay was registered during several flares too. Some spectral peculiarities in the region of 15–21 MeV were first observed in solar flare energy spectrum.     

现场校准试验用便携式γ射线照射装置研制

固定式环境γ辐射剂量率监测仪表是承担环境连续监测任务的主要设备,这类仪表通常不便于拆卸和安装,而且送检周期较长（一周左右）,影响了连续监测点数据的连续性。为了固定式仪表的按期校准,结合蒙卡方法研制了便携式γ射线照射装置,利用PTW剂量计对辐射场进行标定,最后利用便携式照射装置对固定式环境γ辐射剂量率监测仪表进行现场校准实验。     

激光辅助局部电化学沉积的试验研究

在局部电化学沉积加工体系中引入纳秒脉冲激光,利用激光辐照和局部电化学沉积的方法对铜进行三维微结构的沉积试验。分析了激光的热力效应对局部电化学沉积的作用机理。构建了激光辅助局部电化学沉积的试验系统,进行了沉积试验,并利用扫描电子显微镜(Scanning electron microscope,SEM)和X射线能量色散色谱仪对电沉积体进行了检测。试验结果表明激光辅助局部电化学沉积相较于普通的局部电化学沉积,定域性好。随着激光能量的增加,沉积体的高宽比增加,定域性提高。同时,激光还可以减少阴极杂质的吸附,提高沉积体的纯度。     

A study on the resistance performance of epoxy nano-composites under the vacuum ultraviolet irradiation

Irradiation damage effects of the epoxy resin 648 and epoxy nano-composites are studied by means of simulating the vacuum ultraviolet (VUV) irradiation whose wavelength ranges from 5 to 200 nm. Experimental results of the mass loss, SEM and XPS show that nano-TiO₂ particles exhibit better resistance performance under VUV. Comparing with epoxy resin, the epoxy nano-composite brings significantly less mass loss, slighter flexural strength variation and decreasing gas extraction with less gas component varieties after irradiation. What is more, no new carbon peak-value has been found and principle components of O_ls peak-value remain unchanged on the surface.     

辐照环境中ZnO类热控涂层性能

文章研究ZnO类热控涂层在空间综合辐照环境下太阳吸收率(αs)退化的预示模型。利用ZnO类热控涂层的空间综合辐照环境试验数据,对比分析6种数学模型分别拟合出的αs退化预示结果。结果表明,选择合适的预示模型,可以大幅缩短试验时间,利用预示数据就能较准确地反映出αs的退化情况。     

激光驱动典型几何形状碎片运动建模研究

在以往的激光烧蚀驱动移除空间碎片研究中,均假设激光光束覆盖整个所关注的空间碎片。文章提出了焦斑式激光辐照下球体、圆柱体和立方体碎片反喷冲量和运动姿态的计算模型,研究了激光辐照在3种形状碎片不同位置处所产生的反喷冲量和姿态变化规律。结果表明:碎片运动规律与碎片几何形状和激光作用位置有关,当反喷冲量过质心时,碎片获得平动冲量;不过质心时,则会改变碎片的角速度或姿态。研究结果可为激光移除空间碎片研究提供理论参考。     

InxGa1-xAs材料在多结空间太阳电池中的应用进展

In_xGa_(1-x)As材料具有独特的物理特性,可以通过调节In和Ga的组分来改变材料的带隙宽度Eg。该材料自进入多结空间太阳电池领域以来,就受到了广泛的关注。因此,In_xGa_(1-x)As材料有望成为未来多结空间太阳电池领域中的重要研究对象。本文首先介绍了InGaAs材料的生长工艺及其在多结空间太阳电池领域中的应用情况和研究现状,同时讨论了材料的外延生长工艺以获得高质量含InGaAs材料的多结太阳电池。此外,介绍了近年来InGaAs材料在高效多结空间太阳电池领域的研究进展,并对其抗辐照性能进行了简述。大量研究表明:InGaAs材料的使用可以进一步提升多结空间太阳电池的光电转换效率,达到提升卫星有效载荷的目的。     

光子晶体光纤陀螺仪关键技术研究及进展

光子晶体光纤具有辐照不敏感、热敏感度低等特点,可以显著增强光纤陀螺仪的空间环境适应性,并有利于减小光纤陀螺重量、尺寸和功耗。本文分析了光子带隙型光子晶体光纤和折射率导引型光子晶体光纤的特点,详细阐述了光子晶体光纤陀螺仪的原理、关键技术及国内外进展。     

激光与金属材料相互作用的热效应分析

激光与金属材料相互作用的热效应是激光束辐照材料后发生的主要物理现象之一.激光加热使材料温度急剧上升,很快达到材料的熔点.通过使用商业CFD软件FLUENT数值模拟激光辐照金属材料的相互作用,并在一定的假设和边界条件下得到金属材料未熔化之前温度场沿径向和轴向分布情况、气流最高温度的变化和位置的转移、氧化反应和对流换热对热效应的影响.