MSM结构ZnO紫外探测器的制备及光电性能研究

采用磁控溅射方法,在石英衬底上制备了光电性能优良的ZnO紫外探测器。通过紫外光电性能测试、扫描电子显微镜(SEM)观察及X射线衍射(XRD)分析,研究了ZnO紫外探测器的光电特性。结果表明:探测器的光电流高出暗电流近3个数量级,紫外波段的光响应高出可见光波段近2个数量级,所制备ZnO紫外探测器达到了高辐射灵敏度和可见盲特性的要求。     

制导工具误差对导弹射击精度的影响分析

探讨了影响导弹射击精度的主要工具误差系数偏差,建立了导弹惯测组合输出仿真和误差补偿仿真的数学模型。在标准弹道基础上将建立的仿真模型加入导航计算过程,建立了惯测组合工具误差的干扰道模型,并计算分析了不同射向,射程下的工具差系数偏差对导弹薄点的影响,为进一步研究减小制导工具误差的途径打下了基础。     

UV光固化胶粘剂的研制

研制出了一种适用于高档家具玻璃、玻璃工艺器、水晶玻璃，光学玻璃等胶接用的丙烯酸系UV光固化胶粘剂，该胶粘接强度高、耐水性能好，玻璃接头在沸水中煮数十小时不剥离。     

Remote sounding of atmospheric gravity waves with satellite limb and nadir techniques

Recent advances in satellite techniques hold great potential for mapping global gravity wave (GW) processes at various altitudes. Poor understanding of small-scale GWs has been a major limitation to numerical climate and weather models for making reliable forecasts. Observations of short-scale features have important implication for validating and improving future high-resolution numerical models. This paper summarizes recent GW observations and sensitivities from several satellite instruments, including MLS, AMSU-A, AIRS, GPS, and CLAES. It is shown in an example that mountain waves with horizontal wavelengths as short as 30 km now can be observed by AIRS, reflecting the superior horizontal resolution in these modern satellite instruments. Our studies show that MLS, AMSU-A and AIRS observations reveal similar GW characteristics, with the observed variances correlated well with background winds. As a complementary technique, limb sounding instruments like CRISTA, CLAES, and GPS can detect GWs with better vertical but poorer horizontal resolutions. To resolve different parts of the broad GW spectrum, both satellite limb and nadir observing techniques are needed, and a better understanding of GW complexities requires joint analyses of these data and dedicated high-resolution model simulations.     

Ultraviolet images of galaxies from the Optical Monitor on XMM-Newton

A large number of galaxies, both normal and active, have been observed in ultraviolet light by the Optical Monitor on XMM-Newton. These are some of the deepest wide-field ultraviolet images of these galaxies yet obtained, and in many cases the first collected in this waveband. We present images of five active galaxies, and discuss the potential uses of the ultraviolet surface brightness distribution and morphology, in association with X-ray data, for Active Galactic Nuclei, star formation and galaxy evolution studies.     

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.      

R3D-B2 – Measurement of ionizing and solar radiation in open space in the BIOPAN 5 facility outside the FOTON M2 satellite

Solar and space radiation have been monitored using the R3D-B2 radiation risks radiometer-dosimeter on board a recent space flight on the Russian satellite Foton M2 within the ESA Biopan 5 facility mounted on the outside of the satellite exposed to space conditions. The solar radiation has been assayed in four wavelength bands (UV-C, 170–280 nm, UV-B, 280–315 nm), UV-A (315–400 nm) and PAR (photosynthetic active radiation, 400–700 nm). The data show an increasing tumbling rotation of the satellite during the mission. The photodiodes do not show a cosine response to the incident light which has been corrected. After calibration of the signals using the extraterrestrial spectrum, doses have been calculated for each orbit, for each day and for the total mission as basic data for the biological material which has been exposed in parallel in the Biopan facility. Cosmic ionizing radiation has been monitored and separated in 256 deposited energy spectra, which were further used for determination of the absorbed dose rate and flux. Basic data tables were prepared to be used by other Biopan 5 experiments. The paper summarizes the results for the Earth radiation environment at the altitude (262–304 km) of the Foton M2 spacecraft. Comparisons with the predictions of NASA Earth radiation environment experimental models AE-8 and AP-8, and the PSB97 model are also presented, which calculate the fluxes of ionizing radiation from a simulation. AP-8 is a model for trapped radiation.     

空间紫外辐照对高分子材料破坏机理研究综述

高分子材料作为绝缘体和电介质被广泛应用于机电组件、集成电路等各类电子元器件中,其性能的变化将直接影响电子元器件功能的正常实现。空间紫外辐照是造成高分子材料性能退化的重要因素之一。文章介绍了空间紫外辐照的来源及特点,阐述了紫外辐照对高分子材料作用的两种效应,即瞬态效应和累积效应的机理与过程及其对高分子材料性能造成的影响,并提出增强高分子材料耐紫外辐照能力的方法和途径。最后指出需要进一步开展研究工作的方向。