嫦娥五号月面上升和下降段实时轨道确定

针对月球探测中月面上升和下降段的实时轨道确定问题,提出基于三向测量的实时自适应当前统计方法。首先,通过自适应当前统计模型描述探测器月面上升下降过程,其次,综合利用三向数据进行测量更新,最后,通过UKF滤波算法完成实时轨道确定。由于自适应当前统计模型具有良好的适应性,该方法能对探测器月面上升和下降段进行有效定位,通过嫦娥五号探测器实际上升和下降过程数据进行测试,结果表明,文章提出的基于三向测量的实时自适应当前统计方法比传统的几何定位方法具有更好的抗差性,对深空目标探测具有一定的工程应用价值。     

阿里安5的结构材料与工艺的新进展

阿里安５和当前正在使用的阿里安４相比，直径和贮箱容积以及推力都有了极大增加，还提高了可靠性要求。     

以恒星位置为基准的运动平台上测控雷达精度标校技术

利用FK5星表，可以精确实时地计算出恒星位置，用作陆基雷达标校的基准。本文把这种技术推广到运动平台上雷达的精度标校，提出了技术方案和初步的数学模型，给出了试验的解算结果和统计结果。     

CFM56-5B发动机性能衰退评估

发动机性能衰退通常用排气温度裕度EGTM和外界大气温度限制值OATL 来衡量。本文给出了一种CFM56-5B发动机EGTM和OATL的计算方法,可以作为发动机换发的参考。     

N5A飞机中翼前梁缘条LC9型材过时效工艺试验

介绍了ＬＣ９型材过时效工艺试验和过时效及人工时效对比试验情况，从而作出了ＬＣ９型材经过时效处理可装机使用的结论。     

The heart-shaped supernova remnant 3C 391 viewed in multi-bands

Using Chandra X-ray, Spitzer mid-IR, and 1.5 GHz radio data, we examine the spatial structure of SNR 3C 391. The X-ray surface brightness is generally anti-correlative with the IR and radio brightness. The multiband data clearly exhibit a heart-shaped morphology and show the multi-shell structure of the remnant. A previously unseen thin brace-like shell on the south detected at 24 μm is projected outside the radio border and confines the southern faint X-ray emission. The leading 24 μm knot on the SE boundary appears to be partly surrounded by soft X-ray emitting gas. The mid-IR emission is dominated by the contribution of the shocked dust grains, which may have been partly destroyed by sputtering.     

线谱对(LSP)分析在G.729语音编码算法中的应用

本文介绍了线谱对(Linear Spectrum Pair,LSP)分析的基本原理及其在G.729中的应用,同时分析比较了LSP参数与常用的线性预测系数LPC的区别,仿真结果表明,LSP参数的抗干扰能力远比LPC系数的抗干扰能力强。     

Zn粉和Al粉固相扩散形成共晶类组织的研究

在冷压制、热压制等不同工艺条件下制备出块状的Zn 5Al试样 ,得到了更细密的两相相间排列的准共晶组织。用OM ,SEM ,TEM和X射线衍射并结合能谱分析等方法研究了准共晶合金试样在各种实验条件和变形过程中的变化及其有关的界面作用。研究发现 ,原子沿晶界 (相界 )和自由表面的扩散过程在准共晶组织的形成过程中起到了关键性的作用     

An inversion approach for lunar regolith layer thickness using optical albedo data and microwave emission simulation

An approach to inversion of the lunar regolith layer thickness by using multi-channel brightness temperature observation in passive microwave remote sensing is developed. To first make simulation of brightness temperature from the lunar layered media, the lunar regolith layer thickness (d) is proposed being constructed by available lunar DEM (digital elevation mapping) and on site measurements. The physical temperature distribution (T) over the lunar surface is also empirically assumed as a monotonic function of the latitude. Optical albedo of the lunar nearside from the telescopic observation is employed to construct the spatial distribution of the FeO+TiO₂ content (S) in the lunar regolith layer. A statistic relationship between the DEM and S of the lunar nearside is further extended to construction of S of the lunar farside. Thus, the dielectric permittivity (ε) of global lunar regolith layer can then be determined. Based on all these conditions (d,T,ε), brightness temperature of the lunar regolith layer in passive microwave remote sensing, which is planned for China's Chang-E lunar project, is numerically simulated by a parallel layering model using the strong fluctuation theory of random media.Then, taking these simulations with random noise as observations, an inversion method of the lunar regolith layer thickness is developed by using three- or two-channels brightness temperatures. When the S is low, and the four channels brightness temperatures in China's Chang-E project are well distinguishable, the regolith layer thickness and physical temperature of the underlying lunar rock media can be inverted by the three-channels approach. When the S becomes high that the brightness temperature at high frequency channels such as 19.35, 37 GHz are saturated, the regolith layer thickness is alternatively inverted only by the two-channels approach.Numerical simulation and inversion approach in this paper make an evaluation of the performance for lunar passive microwave remote sensing, and for future data calibration and validation.