CAS-1 lunar soil simulant

Lunar soil simulant is a geochemical reproduction of lunar regolith, and is needed for lunar science and engineering researches. This paper describes a new lunar soil simulant, CAS-1, prepared by the Chinese Academy of Sciences, to support lunar orbiter, soft-landing mission and sample return missions of China’s Lunar Exploration Program, which is scheduled for 2004–2020. Such simulants should match the samples returned from the Moon, all collected from the lunar regolith rather than outcrops. The average mineral and chemical composition of lunar soil sample returned from the Apollo 14 mission, which landed on the Fra Mauro Formation, is chosen as the model for the CAS-1 simulant. Source material for this simulant was a low-Ti basaltic scoria dated at 1600 years from the late Quaternary volcanic area in the Changbai Mountains of northeast China. The main minerals of this rock are pyroxene, olivine, and minor plagioclase, and about 20–40% modal glass. The scoria was analyzed by XRF and found to be chemically similar to Apollo 14 lunar sample 14163. It was crushed in an impact mill with a resulting median particle size 85.9 μm, similar to Apollo soils. Bulk density, shear resistance, complex permittivity, and reflectance spectra were also similar to Apollo 14 soil. We conclude that CAS-1 is an ideal lunar soil simulant for science and engineering research of future lunar exploration program.     

基于GJB289A标准的通用总线数据分析

基于GJB289A总线标准协议,采用先进的数据分析解算算法,对总线记录仪记录的总线数据文件进行分析,系统支持多粒度、多种方式的数据分析和显示功能。系统与ICD采用自动对接,针对不同型号提供统一的分析接口;采用C/S模式的系统结构,既满足多用户同时使用,又满足不同型号同时在线分析,真正实现了系统的通用性。     

嫦娥一号卫星双轴天线轨迹规划

针对嫦娥一号卫星双轴天线指向地球的控制要求,给出双轴天线框架角的计算方法．根据地球可见条件及双轴天线转动角度和角速度的限制。确定星上双轴天线自主跟踪地球的范围．最后,在轨飞行试验结果验证了该方法的有效性．     

嫦娥一号卫星热控设计中热管的应用及验证

为克服由于月球热环境的特殊性给热控设计带来的困难,尤其是卫星度过月食的极端状态条件,首次采用了舱外两舱热耦合热管、相变材料热管技术,为最终嫦娥一号卫星热控状态满足总体的技术要求发挥了关键作用。由于两舱热耦合技术的采用,两舱的热能量得到了相互补偿,因此减少了整星散热面,减少了热补偿功率需求,提高了月食结束时蓄电池的温度,使热控技术方案成为相对优化的方案。文章对热管技术在嫦娥一号卫星热控设计中的应用进行了总结,并给出了热分析及热平衡。     

“实践九号”A卫星光学遥感图像杂散光噪声去除

杂散光是影响卫星光学遥感图像像质的重要因素,严重时会在图像上形成明暗的杂散光条纹噪声,降低图像的对比度和清晰度。文章针对“实践九号”A（SJ-9A）卫星光学遥感图像存在的杂散光噪声现象,设计了一种基于成像载荷焦面入射杂散光空间分布特征的遥感图像杂散光条纹噪声去除方法,通过测量杂散光在推扫遥感图像上的空间分布特征,建立杂散光分布特征模型,采用分块自适应算法进行杂散光噪声滤波,消除SJ-9A遥感图像上随时空变化的杂散光条纹噪声。杂散光噪声去除后图像整体色调均匀,无条带噪声,满足CCD/TDI-CCD推扫遥感图像辐射校正精度（广义噪声）优于5%的指标要求。     

基于时间误差补偿的HJ-1C卫星几何定位改进

利用距离多普勒算法对 HJ-1C（“环境一号”C）卫星图像进行定位,其初始定位精度为1100~1400m,不能很好地满足实际应用的需要。进一步分析后发现,HJ-1C卫星图像几何定位误差主要分布在方位向,通过对影响HJ-1C卫星几何定位精度的因素进行分析,得出合成孔径雷达（Synthetic Aperture Radar, SAR）时间误差是影响几何定位的关键因素,因此文章提出通过时间误差补偿提高HJ-1C卫星几何定位精度。该方法首先计算SAR时间误差,然后对SAR载荷时间进行补偿,最后利用距离多普勒算法进行定位,并对HJ-1C卫星图像进行了验证。结果表明,HJ-1C卫星定位精度提高到300m左右,得到了有效的改进。     

《爱犬弗拉狮传》的“戏仿”实验

研究伍尔夫颠覆传统传记的"戏仿"实验。在《爱犬弗拉狮传》中选择一条宠物狗作为传主,运用娴熟的操纵视角手法,以"戏仿"的方式,颠覆文坛沿袭的维多利亚传记传统。这种高超的叙事技巧证明伍尔夫不仅是一个艺术的讲故事者,还是一个才华横溢的维多利亚传记传统的反叛者。     

Computations of unsteady transonic flow over airfoil at low Reynolds number

Transonic flow over a thin airfoil at low Reynolds number was studied numerically by directly solving two-dimensional full Navier-Stokes equations through 5th order weighted essentially non-oscillatory(WENO) scheme without using any turbulence model.A series of distinguished unsteady phenomena for a thin 2-D transonic airfoil flow were presented.Due to continuous adverse pressure gradient in the subsonic flow downstream of the sonic line, the unsteady separated boundary layer with main vortex and secondary vortex was developed at the rear of the airfoil.At the trailing edge,the vortex-shedding was characterized by periodical connection of the main vortex and secondary vortex on the other side of the airfoil.The unsteady separation and vortex-shedding occurred with the same period.On the airfoil surface,the average pulse pressure related to the unsteady supersonic region was obviously smaller than that related to the vortex-shedding at the trailing edge.With the attack angle increasing from 0° to 2°, the frequency of vortex-shedding decreases about 4.2%.At last, the turbulence intensity and many second-order statistics in the wake region were investigated.      

F1方程式赛车后升力翼的气动特性

以比例为1∶3的F1方程式赛车后升力翼为研究对象,研究了后升力翼攻角变化对F1方程式赛车气动阻力和气动升力的影响规律.在攻角为12°时,气动升力与气动阻力的比值的绝对值达到最大,此攻角就是F1方程式赛车后升力翼的最佳攻角,模型风洞试验验证了这一结论.      

GPS伪随机码畸变的建模与分析

建立了全球卫星定位系统(GPS)卫星C/A码畸变数学模型,推导了畸变后的C/A码的相关函数,在Matlab软件中进行仿真。结果表明:该模型能合理解释SVN19卫星的测距码畸变故障,并可作为未来伪随机信号畸变的一个合理模型,为导航信号的完好性监测提供理论支持。