采用串列静电加速器进行单粒子效应模拟试验研究

本文描述了采用ＨＩ－１３串列静电加速器进行单粒子效应模拟试验的试验系数、试验方法和试验条件，给出了８０Ｃ３１单片机单粒子效应模拟试验结果；根据试验结果，采用ＣＲＥＭＥ程序对８０Ｃ３１单片机在三类不同轨道卫星上的单粒子翻转率进行了预计。     

美国光学特性测量技术发展情况及特点

简要介绍了美国地基、空基、天基光学特性测量技术的发展情况，对其在光学特性测量技术领域发展的特点给予了分析、总结。     

磁屏蔽装置与磁场模拟器的耦合分析

地磁导航半实物仿真是地磁导航从理论走向工程应用的关键环节,而地磁场环境仿真技术是地磁导航由计算机仿真过渡到半实物仿真的桥梁。针对地磁场环境仿真系统中磁屏蔽装置与其内部磁场模拟器的耦合问题,采用仿真分析与实验验证相结合的方法,利用Ansoft Maxwell仿真软件设计仿真实验对二者的耦合关系进行了探索性研究,并基于小型地磁场环境仿真系统对仿真得到的结论进行了实验验证。仿真和实验结果均表明:磁场模拟器在大电流强磁场的工作情况下会对磁屏蔽装置造成严重的磁化,进而会影响其屏蔽效果;磁屏蔽装置不会影响磁场模拟器的线性度和均匀性,但是会增大轴线中心点附近的磁场值;磁屏蔽装置会使磁场模拟器的电感增大,从而使实时性变差。研究结论可以为地磁场环境仿真系统的设计提供理论依据。      

煤油-氧火焰中铁的辐射光谱实验研究

为了对羽流激波中金属光谱特性进行研究,用煤油-氧火焰气体模拟煤油-氧发动机的羽流,以二茂铁溶于煤油模拟发动机材料铁的磨损,给出不同混合比下铁在火焰中辐射光谱的实验与仿真结果.实验光谱数据随铁的浓度不同而变化,理论光谱与实验结果吻合较好,验证了羽流中金属原子辐射光谱的仿真程序.为基于羽流光谱分析的发动机故障诊断研究奠定了实验与理论基础.     

Surface temperatures at the nearside of the Moon as a record of the radiation budget of Earth’s climate system

Understanding the balance between incoming radiation from the Sun and outgoing radiation from Earth is of critical importance in the study of climate change on Earth. As the only natural satellite of Earth, the Moon is a unique platform for the study of the disk-wide radiation budget of Earth. There are no complications from atmosphere, hydrosphere, or biosphere on the Moon. The nearside of the Moon allows for a focus on the solar radiation during its daytime, and on terrestrial radiation during its nighttime. Additionally, lunar regolith temperature is an amplifier of the terrestrial radiation signal because lunar temperature is proportional to the fourth square root of radiation as such is much more sensitive to the weak terrestrial radiation in nighttime than the strong solar radiation in daytime. Indeed, the long-term lunar surface temperature time series obtained inadvertently by the Heat Flow Experiment at the Apollo 15 landing site three decades ago may be the first important observation from deep space of both incoming and outgoing radiation of the terrestrial climate system. A revisit of the lunar surface temperature time series reveals distinct characteristics in lunar surface daytime and nighttime temperature variations, governed respectively by solar and terrestrial radiation.     

"闪晕"的电场结构和光辐射的时变模拟

用时变的2-D准静电场模型,研究了由雷暴放电产生的静电场在中间层-低电离层的空间结构、时延、持续时间、向下传播的速度以及静电场引起的大气电离和光辐射．研究表明,由静电场引起的氮分子第一个正波段光辐射的时空特征与观测到的“闪晕”时空特征基本一致．     

An exploration of the effectiveness of artificial mini-magnetospheres as a potential solar storm shelter for long term human space missions

If mankind is to explore the solar system beyond the confines of our Earth and Moon the problem of radiation protection must be addressed. Galactic cosmic rays and highly variable energetic solar particles are an ever-present hazard in interplanetary space.     

Electrostatic space radiation shielding

For the success of NASA’s new vision for space exploration to Moon, Mars and beyond, exposures from the hazards of severe space radiation in deep space long duration missions is ‘a must solve’ problem. The payload penalty demands a very stringent requirement on the design of the spacecrafts for human deep space missions. The exploration beyond low Earth orbit (LEO) to enable routine access of space will require protection from the hazards of the accumulated exposures of space radiation, Galactic Cosmic Rays (GCR) and Solar Particle Events (SPE), and minimizing the production of secondary radiation is a great advantage. There is a need to look to new horizons for newer technologies. The present investigation revisits electrostatic active radiation shielding and explores the feasibility of using the electrostatic shielding in concert with the state-of-the-art materials shielding and protection technologies. The full space radiation environment has been used, for the first time, to explore the feasibility of electrostatic shielding. The goal is to repel enough positive charge ions so that they miss the spacecraft without attracting thermal electrons. Conclusions are drawn for the future directions of space radiation protection.     

A noise attenuation method for medium-energy electron measurements in the radiation belt

From the viewpoint of plasma particle measurements in the radiation belt, background noise is a serious problem. High-energy particles penetrating the sensor shielding generate spurious signals, and their count rate often can be comparable to the true signals. In order to attenuate such background noise during medium-energy (5–83 keV) electron measurements, we propose the double energy analyses (DEA) method. DEA is conducted by a combination of an electrostatic analyser (ESA) and avalanche photo-diodes (APDs); ESA and APD independently determine the energy of each incoming particle. By using the DEA method, therefore, the penetrating particles can be rejected when the two energy determinations are inconsistent; spurious noise are caused only when the deposited energy at an APD is by chance consistent with the measured energy by ESA. We formulate the noise count rate and show the advantage of DEA method quantitatively.     

计算机电磁泄漏测试及防护措施

论述了计算机电磁泄漏的危害及测试的意义,介绍了测试系统的组成,对某国产微型计算机进行了测试,并对其测试数据进行了分析,提出了行之有效的防护措施。