基于支持度的MEMS陀螺信息融合方法

为了解决微机械电子系统(MEMS, micro electronic mechanical system) 惯性器件测量准确度低、噪声大、长时间单独使用导航误差积累大等缺点,提出了一种MEMS陀螺阵列结构设计,在完成微型惯性测量单元(MIMU, micro inertial measurement unit)的标定后,采用基于支持度的信息融合方法对陀螺阵列输出进行信息融合。试验结果表明：该结构设计和信息融合方法能够有效的提高MIMU的测量准确度,具有一定的工程应用价值。     

Development of thermal sensors and drilling systems for lunar and planetary regoliths

We consider some novel concepts for thermal properties experiments aboard lunar landers or rovers, that may lead to an improved understanding of both the structure of the lunar near surface layers and the lunar thermal history. The new instruments could be developed using the experience and heritage from recently developed systems, like the Rosetta Lander thermal conductivity experiment MUPUS and existing designs used for terrestrial measurements of thermal conductivity. We describe shortly the working principle of such sensors and the main challenges faced when using them in the airless regolith layers of the Moon or other airless bodies. In addition new concepts to create appropriate drill holes for thermal and other measurements in the lunar regolith are discussed.     

Relative amplitude of the total electron content variations depending on geomagnetic activity

We developed a method of estimation of a relative amplitude dI/I of the total electron content (TEC) variations in the ionosphere as deduced from the data of the global GPS receivers network. To obtain statistically significant results we picked out three latitudinal belts provided in the Internet by the maximum number of GPS sites. They are high-latitudinal belt (50–80°N, 200–300°E; 59 sites), mid latitude belt (20–50°N, 200–300°E; 817 sites), and equatorial belt (±20°N, 0–360°E; 76 sites). The results of the analysis of the diurnal and latitudinal dependencies of dI/I and dI/I distribution probability for 52 days with different levels of geomagnetic activity are presented. It was found that on average the relative amplitude of the TEC variations varies within the range 0–10% proportionally to the value of the K_p geomagnetic index. In quiet conditions the relative amplitude dI/I of the TEC variations at night significantly exceeds the daytime relative amplitude. At high levels of magnetic field disturbances, the geomagnetic control of the amplitude of TEC variations at high and middle latitudes is much more significant than the regular diurnal variations. At the equatorial belt, on average, the amplitude of TEC variations in quiet and disturbed periods almost does not differ. The obtained results may be useful for development of the theory of ionospheric irregularities.     

Roe格式中不同类型熵修正性能分析

针对Roe格式中较为流行的3类熵修正:Muller型、Harten-Yee型和Harten-Hyman型熵修正,从理论分析入手, 辅以Euler方程为控制方程的激波管问题,前台阶流动和运动激波的双马赫反射3个数值实验,对不同熵修正的性能做了深入研究,得出如下结论: Muller型和Harten-Yee型熵修正方法作用于激波和非物理的膨胀激波2种情况:激波情况下引入的数值耗散,能根本改善"Carbuncle"现象,膨胀激波时其数值粘性也足以使膨胀激波得以耗散;而类Harten-Hyman型熵修正只对膨胀过程起修正作用,对激波情况无效,不能改善"Carbuncle"现象,该类熵修正的数值粘性较小,不足以使膨胀过程正确求解;直接采用 δ 值代替特征值的特征值修正方法效果好于传统的特征值修正方法.     

不确定载荷下的桁架结构拓扑优化

对带有不确定扰动载荷的桁架结构拓扑优化问题进行了研究.将不确定载荷表示成有界凸集,从而把不确定性问题转化为一个确定性问题.构造了凸集载荷下以体积为约束的柔度最小化模型,该优化模型的实质是在高维椭球内计算最大柔度最小问题.由于采用传统优化模型存在计算上的困难,对凸集载荷进行了数学处理,并据此构造了半定规划形式的优化模型以便求解.优化结果相对于给定载荷的刚度虽然略低,但对不确定的扰动载荷却具有一定的承载能力.算例表明通过半定规划法构造的考虑扰动载荷作用下的优化结果鲁棒性较佳,结构形式更接近于实际工程结构.     

基于PCI总线的主从式多轴控制器开发

针对运动控制的高精度要求,介绍了一种基于PCI(Peripheral Component Interconnect)总线的实时多轴控制系统.为了在执行复杂任务时,减少主机的工作量以及充分利用数字信号处理器(DSP,Digital Signal Processor)的数字处理能力,多轴控制器采用了主从控制结构.这种控制器还可以根据用户的需要使用串行通讯控制来代替PCI总线控制.控制器硬件的研发主要集中在多轴控制器、PCI总线接口电路和PCI局部总线的控制逻辑电路上,这些是设计控制器的关键技术.通过一个三自由度机器人沿一个空间螺旋轨迹运动的实例验证,所研发的多轴控制器可以实现具有准实时性能的高精度协调运动控制.      

N2O单组元微推力器性能分析及试验

N₂O单组元微推进是当前微推进领域的一个热点问题.在N₂O催化分解热力计算的基础上开展了对N₂O单组元微推力器比冲性能影响因素的分析,分析结果表明微推力器比冲与N₂O分解效率及喷管扩张比有密切关系.所开展的亚牛级N₂O单元微推力器催化分解试验结果表明所设计N₂O单元推力器能在250℃初温条件下启动,初步验证了N₂O单元微推力器的可行性;也揭示了推力室结构及床载大小对亚牛级N₂O单元微推力器性能的影响,为进一步的结构及试验设计提供了参考.     

The IMPACT Solar Wind Electron Analyzer (SWEA)

SWEA, the solar wind electron analyzers that are part of the IMPACT in situ investigation for the STEREO mission, are described. They are identical on each of the two spacecraft. Both are designed to provide detailed measurements of interplanetary electron distribution functions in the energy range 1～3000 eV and in a 120°×360° solid angle sector. This energy range covers the core or thermal solar wind plasma electrons, and the suprathermal halo electrons including the field-aligned heat flux or strahl used to diagnose the interplanetary magnetic field topology. The potential of each analyzer will be varied in order to maintain their energy resolution for spacecraft potentials comparable to the solar wind thermal electron energies. Calibrations have been performed that show the performance of the devices are in good agreement with calculations and will allow precise diagnostics of all of the interplanetary electron populations at the two STEREO spacecraft locations.     

基于离散数据点的变壁厚叶身参数化设计

在原始截面离散数据点的基础上,给出了面向工程实际的中弧线几何造型方法和基于离散数据点的内形曲线参数化方法;深入分析了UG(Unigraphic)系统参数化造型的实质;给出了可行的参数化方案;结合面向对象的思想和创成式的建模方式,实现了变壁厚叶身参数化设计.该模块基于UG/OpenAPI接口,采用即时记录数据点和标记回溯点的方式,在交互中可以实时动态修改,达到"所见即所得"的效果,并在实际应用中得到有效验证.