A laboratory study on the thermally induced transformation of hydrogen cyanide (HCN) to the cyanogen anion (CN) in Solar System analog ices

Mixtures of molecular nitrogen and methane have been identified in numerous outer Solar Systemices including the icy surfaces of Pluto and Triton. We have simulated the interaction of ionizing radiation in the Solar System by carrying out a radiolysis experiment on a methane – molecular nitrogen ice mixture with energetic electrons. We have identified the hydrogen cyanide molecule as the most prominent carbon–nitrogen-bearing reaction product formed. Upon warming the irradiated sample, we followed for the first time the kinetics and temporal evolution of the underlying acid–base chemistry which resulted in the formation of the cyanide ion from hydrogen cyanide. On the surfaces of Triton and Pluto and on comets in Oort’s cloud this sort of complex chemistry is likely to occur. In particular, hydrogen cyanide can be produced in low temperature environments (Oort cloud comets) and may be converted into cyanide ions once the comets reach the warmer regions of the Solar System.     

PAMELA observational capabilities of Jovian electrons

PAMELA is a satellite-borne experiment that has been launched on June 15th, 2006. It is designed to make long duration measurements of cosmic radiation over an extended energy range. Specifically, PAMELA is able to measure the cosmic ray antiproton and positron spectra over the largest energy range ever achieved and will search for antinuclei with unprecedented sensitivity. Furthermore, it will measure the light nuclear component of cosmic rays and investigate phenomena connected with solar and earth physics. The apparatus consists of: a time of flight system, a magnetic spectrometer, an electromagnetic imaging calorimeter, a shower tail catcher scintillator, a neutron detector and an anticoincidence system. In this work a study of the PAMELA capabilities to detect electrons is presented. The Jovian magnetosphere is a powerful accelerator of electrons up to several tens of MeV as observed at first by Pioneer 10 spacecraft (1973). The propagation of Jovian electrons to Earth is affected by modulation due to Corotating Interaction Regions (CIR). Their flux at Earth is, moreover, modulated because every 13 months Earth and Jupiter are aligned along the average direction of the Parker spiral of the Interplanetary Magnetic Field.PAMELA will be able to measure the high energy tail of the Jovian electrons in the energy range from 50 up to 130 MeV. Moreover, it will be possible to extract the Jovian component reaccelerated at the solar wind termination shock (above 130 MeV up to 2 GeV) from the galactic flux.     

用于识别两颗故障卫星的RAIM算法

提出了一种可以识别两颗故障卫星的接收机自主完好性监测算法.将最优奇偶矢量法应用于两颗故障卫星识别,指出由于故障偏差可能会抵消而使得正确识别率较低.对最优奇偶矢量法进行了改进,利用对单颗卫星故障敏感的最优奇偶矢量对所有可能的两颗故障卫星组合分别构造两个新的奇偶矢量,用于两颗故障卫星的检测和识别.计算机仿真结果显示,改进后的算法与直接利用最优奇偶矢量法相比,可以显著提高两颗故障卫星正确识别率,识别率可超过90%.同时,改进算法的奇偶矢量构造方法简单,计算量将减少90%以上,更有利于工程实现.      

组合卫星接收机中的选星算法

分析了五阶矩阵的行列式值与5颗星GDOP(Geometry Dilution of Precision)值的关系,并由此提出了一种用于双卫星星座组合接收机(如GPS(Global Position System)和BD2(BeiDou2)组合接收机)中的选星算法——组合优选法.该方法首先选出行列式绝对值最大的几种组合,然后根据需要对每种组合从其余可见星中选出几颗最优星,最后根据GDOP最小原则从这几种组合中选取最终结果.计算机仿真结果显示该方法与直接利用GDOP选星相比,95％以上的GDOP相对比值小于5％,而计算量减小40％以上.      

限制励磁方法在无刷交流发电机数字电压调节器中的应用

分析了限制励磁电流功能对无刷交流发电机加载过渡过程的影响,得到了设置励磁电流限制值的方法。采用了曲线拟合的方法对变速无刷交流发电机的励磁电流限制值进行了设置,而且拟合公式是与理论推导相一致的。按照本文的励磁电流限制值拟合方法可以保证无刷交流发电机在整个转速范围内都有良好的加载动态性能。     

基于试飞任务单的轨迹仿真问题研究

阐述了基于试飞任务单的试飞轨迹仿真生成软件系统在辅助试飞管理中的重要作用,对该软件开发中所涉及到的一些新的问题和方法进行了研究。建立了带电传操纵系统飞机的数学模型,并针对试飞轨迹仿真生成中的逆问题,提出了一种基准控制带反馈调节的方法。简要介绍了轨迹仿真生成软件与任务单管理数据库软件的接口设计,对仿真结果进行了动态显示处理。     

企业的知识管理及其措施探讨

知识经济时代已经到来,适应知识经济的企业管理方式正从工业社会的生产管理向知识管理和创新管理转变。笔者对企业知识管理的概念进行了分析,并探讨企业进行知识管理的具体措施。     

航天器运输包装箱仿真验证平台技术研究

针对数量有限的物理跑车试验无法满足减振与保温性能测试需求的问题,提出一套航天器运输包装箱动力学与热学仿真验证方法,包括:建立适用于包装箱系统的刚柔耦合多体动力学系统,通过结合线路条件测试生成的动力学系统外部激励,实现减振性能虚拟跑车测试;建立基于计算流体力学的包装箱热学模型,通过模拟自然对流和空调控制,实现包装箱保温性...     

高背压等离子点火器及其液体燃料点火特性实验研究

航天应用的液体火箭发动机及燃烧型加热器燃烧室室压高、燃料流量大、温度低、有重复启动需求,实现安全可靠点火的难度较大.针对这些需求,研究了一种采用高背压设计的电弧等离子体点火器.实验研究了Ar,N2气体工质在高进气压力下的伏安特性,发现N2在宽压力范围内适用于点火.发射光谱分析表明,在高达数MPa的进气压力下,Ar,N2...