Earthshine and Asteroseismology Telescope (East) Network

Several automated optical telescopes have been setup at appropriate longitudes around the globe to study earthshine variations and asteroseismology. The first telescope has been setup at Teide Observatory, Tenerife, Spain in October 2004. The intensity of earthshine relates to the average of Earth’s albedo, and in turn relates to the global temperature of the Earth. A global network is necessary because each site can measure the earthshine reflected from only a part of the Earth. The network will also be used for asteroseismology study. It can measure photometric variations of pulsating stars. The long-term and continuous measurements allow the accurate determination of mode frequencies of stellar pulsations, which provides information on the properties of stellar interior.     

硼酸盐玻璃中稀土离子的发光研究

应用荧光光谱、红外振动光谱等研究了在可见光区发光的Ｐｒ（３＋），Ｓｍ（３＋），Ｅｕ（３＋），Ｔｂ（３＋），Ｄｙ（３＋），Ｅｒ（３＋）和Ｔｍ（３＋）等镧系稀土离子在硼酸盐玻璃中的发光行为，系统地分析了稀土离子在硼酸盐玻璃基质中的激发谱和发光谱特性。     

太空中相继升起近80颗中国的人造地球卫星——庆贺中国航天事业创建50周年

回顾了中国自主发展人造地球卫星的历程,以此庆贺中国航天事业创建50周年。     

Acceleration of interplanetary pick-up ions and anomalous cosmic rays

It may not be doubted anymore that anomalous cosmic rays (ACRs) are produced in the heliosphere from interplanetary pick-up ions through their acceleration at the solar wind termination shock. However, there is no general agreement in the community of heliospheric researchers concerning the mechanism of injection of the pick-up ions into the shock acceleration. We discuss here three possible ways for pick-up ions to be involved into the acceleration process at the termination shock: (1) preacceleration of pick-up ions in the whole region from the Sun up to the termination shock by solar wind turbulences and interplanetary shock waves, (2) local preacceleration of pick-up ions in a vicinity of the termination shock by shock surfing, and (3) formation of high-velocity tails in pick-up ion spectra consisting of secondary pick-up ions which are produced in the supersonic solar wind due to ionization of energetic neutral atoms entering from the inner heliosheath.     

Avoid online radiation risk: Theoretical simulation of chromosome breaks in cells exposed to heavy ions

In this study, we report an easy and quick method on simulating chromosome breaks in cells exposed to heavy charged particles. The theoretical value of chromosome break was calculated, and validated comparison with experimental value by using premature chromosome condensation technique. A good consistency was found between theoretical and experimental value. This suggested that higher relative biological effectiveness of heavy ions was closely correlated with its physical characteristics. Also, a safe approach on predicting chromosome breaks in cells exposed to heavy ions at off-line environment can be considered. Furthermore, three key factors influencing the theoretical simulation was investigated and discussed.     

Erosion of a Polyimide Material Exposed to Simulated Atomic Oxygen Environment

Oxygen plasma source generated by thermal cathode filament discharge has been used to study the erosion process of polyimide (PI) materials in atomic oxygen (AO) environment, and their mass loss, surface morphology and surface chemical compositions have been examined by scanning electron microscope (SEM) and X-ray photoelectron spectroscopy (XPS) after exposure to incremental AO flux. The data indicate that the physical adsorption of AO at the samples' surface results in the increase of oxygen concentration when polyimide is exposed to AO flux. Then selective chemical reactions of groups of polyimide materials with AO yield volatile organic compounds, sample mass loss is on linear increase and carpet-like surface morphology forms. In the initial exposure to AO, the reaction occurs mainly between AO and carbon in specific location of aromatic ring, then the reaction rate of C=O groups gradually increases. After AO exposure, the oxygen concentration increases while nitrogen and carbon concentration decreases. Reaction rate of groups containing nitrogen is slower compared with carbon and oxygen.     

ATC计算机系统的地线系统及机房防火措施

在计算机系统的接地系统中,一些问题至今尚无定论,本文结合几个计算机系统安装调试的经验,及现有的ATC雷达模拟系统实体,就机房屏蔽地线、防雷击地线、交流地线、系统地线给予介绍和简单的论述,并给出一些经验值,还说明了直流地悬空的危害和地桩的埋设方法。另外,简要介绍了机房的防火设施,以便有关单位参考。     

AerMet100钢的研究与发展

以AerMet100钢专利和AMS标准的变迁为基础,结合近年来国外AerMet100钢研究内容和材料院相关的研究工作,理出提高AerMet100钢断裂韧度研究的思路.不断提高纯洁度是AerMet100钢断裂韧度提高的重要条件之一;通过多元微量稀土元素改变杂质元素的状态和空间分布,可以有效减少杂质元素对断裂韧度的危害;热处理形成的稳定的逆转变奥氏体对断裂韧度起到积极作用.     

小卫星主动磁控制地球捕获姿态控制系统设计

分析了小卫星捕获阶段的客观条件要求,重力梯度杆的指向要求,捕获阶段视为大角度机动问题,采用欧拉动力学和四元数方法描述,建立小卫星捕获阶段的动力学模型。控制器采用大角度机动拟 PD控制,拟PD控制器参数采用了简化分析和经验调试设计,同时分析设计了磁力矩器的磁偶极子,最后给出某小卫星姿态捕获仿真结果,经过几个轨道周期后可以实现一定精度的对地捕获,验证了本文的设计方法的可行性。     

灯丝放电磁场约束型原子氧效应地面模拟试验设备

介绍了用于原子氧剥蚀效应研究的灯丝放电磁场约束型地面模拟设备 ( IFM)的构成及工作原理,简单阐述了装置的运行测量结果,分析了等离子体参数随试验条件的变化趋势。并用 IFM设备对 Kapton空间用材料进行了地面模拟试验,试验结果与国外空间飞行暴露试验结果相似