多层机匣的包容性数值仿真研究

采用瞬态非线性有限元分析方法对多层机匣的包容性进行了数值仿真研究,对比分析了不同层数机匣在相同撞击条件下的位移、塑性应变和能量的变化,以及同层数机匣有间隙与无间隙时的包容情况。仿真结果表明：同厚度的不同层数机匣,层数越多包容效果越好;对于同层数机匣,层间无间隙机匣的包容效果优于有间隙机匣的。     

可展桁架天线形面精度理论分析

针对可展桁架天线杆件多和转动铰多的特点, 研究杆件加工公差和转动铰间隙对天线反射面精度和重复展开精度的影响. 根据杆件加工公差和转动铰间隙发生的随机性, 建立相应的随机数据模型和Monte-Carlo随机有限元模型, 计算杆件加工公差和转动铰间隙所引起的天线反射面精度误差. 研究表明, 间隙所引起的反射面精度误差远大于杆件公差所引起的误差, 并且天线重复展开精度差值不宜忽视.      

直升机主桨叶的鸟撞有限元数值模拟

以某型直升机主桨叶为例,使用瞬态动力学分析软件(MSC.Dytran),采用先进的任意拉格朗日-欧拉(ALE)流固耦合算法,进行鸟撞过程的数值模拟.模拟结果表明:撞击过程中的最大应力达到199MPa,没有超出桨叶材料的屈服极限.研究结果为桨叶的抗鸟撞损伤设计提供了参考.      

基于虚拟仪器技术的微波测量仿真系统的设计与实现

该系统根据手动测量原理，将传统的微波测量线及相关的微波测量系统在Labview7环境中进行仿真。利用它可实现多种微波参数的仿真测量，并具有图文并茂、生动直观、价格低廉等特点，为微波实验教学及实际应用创造良好的条件。     

基于紫外敏感器和星敏感器的卫星自主导航

卫星利用紫外敏感器和星敏感器进行自主导航的方法中地心矢量的测量精度是影响导航精度的重要因素之一,而地心矢量的测量又受到地球扁率的影响。在考虑地球扁率的前提下,研究了地球扁率对地心矢量测量的影响,给出了基于卫星姿态的地心矢量的补偿方法。仿真结果表明该补偿方法具有较高的补偿精度,并且能有效地提高卫星自主导航精度。     

Plasmaspheric Density Structures and Dynamics: Properties Observed by the CLUSTER and IMAGE Missions

Plasmaspheric density structures have been studied since the discovery of the plasmasphere in the late 1950s. But the advent of the Cluster and Image missions in 2000 has added substantially to our knowledge of density structures, thanks to the new capabilities of those missions: global imaging with Image and four-point in situ measurements with Cluster. The study of plasma sources and losses has given new results on refilling rates and erosion processes. Two-dimensional density images of the plasmasphere have been obtained. The spatial gradient of plasmaspheric density has been computed. The ratios between H⁺, He⁺ and O⁺ have been deduced from different ion measurements. Plasmaspheric plumes have been studied in detail with new tools, which provide information on their morphology, dynamics and occurrence. Density structures at smaller scales have been revealed with those missions, structures that could not be clearly distinguished before the global images from Image and the four-point measurements by Cluster became available. New terms have been given to these structures, like “shoulders”, “channels”, “fingers” and “crenulations”. This paper reviews the most relevant new results about the plasmaspheric plasma obtained since the start of the Cluster and Image missions.     

CLUSTER and IMAGE: New Ways to Study the Earth’s Plasmasphere

Ground-based instruments and a number of space missions have contributed to our knowledge of the plasmasphere since its discovery half a century ago, but it is fair to say that many questions have remained unanswered. Recently, NASA’s Image and ESA’s Cluster probes have introduced new observational concepts, thereby providing a non-local view of the plasmasphere. Image carried an extreme ultraviolet imager producing global pictures of the plasmasphere. Its instrumentation also included a radio sounder for remotely sensing the spacecraft environment. The Cluster mission provides observations at four nearby points as the four-spacecraft configuration crosses the outer plasmasphere on every perigee pass, thereby giving an idea of field and plasma gradients and of electric current density. This paper starts with a historical overview of classical single-spacecraft data interpretation, discusses the non-local nature of the Image and Cluster measurements, and emphasizes the importance of the new data interpretation tools that have been developed to extract non-local information from these observations. The paper reviews these innovative techniques and highlights some of them to give an idea of the flavor of these methods. In doing so, it is shown how the non-local perspective opens new avenues for plasmaspheric research.     

我国利率市场化改革的难点与对策

利率市场化是麦金农和肖金融发展理论针对发展中国家的金融抑制问题提出的重要措施之一.实现利率市场化,需要具备一些基本的条件.我国经济发展水平较低,金融市场发展的不平衡和金融监管滞后,金融制度的不完善以及宏观经济环境的不稳定等因素是我国利率市场化改革的难点.进一步推进利率市场化改革,需要从多方面努力,发展市场经济,提高企业的竞争力;完善金融市场,健全金融监管体系;完善企业金融制度,形成合理的利率形成机制;维护良好的宏观经济运行环境,减轻通胀压力.     

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.     

几何代数域内的光流场改进算法

提山了一种新的光流场计算方法：首先,在几何代数域内推导了光流约束方程的新形式;然后,在速度场平滑的基础上,通过求解关于初值问题的热传导方程求解光流场;最后,给出光流场的数值解和仿真结果。实验证明此方法是有效的。