用Pro/E进行圆柱齿轮的三维参数化特征造型设计

论文介绍了一种基于Pro／Engineer的齿轮三维实体特征造型和利用Program模块实现齿轮的参数化设计方法，可以方便地进行齿轮的二次开发，提高设计效率。     

Characteristics and accuracies of the GRACE inter-satellite pointing

For almost 10 years, the Gravity Recovery and Climate Experiment (GRACE) has provided information about the Earth gravity field with unprecedented accuracy. Efforts are ongoing to approach the GRACE baseline accuracy as there still remains an order of magnitude between the present error level of the gravity field solutions and the GRACE baseline. At the current level of accuracy, thorough investigation of sensor related effects is necessary as they are one of the potential contributors to the error budget. In the science mode operations, the twin satellites are kept precisely pointed with their KBR antennas towards each other. It is the task of the onboard attitude and orbit control system (AOCS) to keep the satellites in the required formation. We analyzed long time series of the inter-satellite pointing variations as they reflect the AOCS performance and characteristics. We present significant systematic effects in the inter-satellite pointing and discuss their possible sources. Prominent features are especially related to the magnetic torquer characteristics, star cameras’ performance and KBR antenna calibration parameters. The relation between the magnetic torquer attitude control and the Earth magnetic field, impact of the different performance of the two star camera heads on the attitude control and the features due to uncertainties in the calibration parameters relating the star camera frame to K-frame are discussed in detail. Proper understanding of these effects will help to reduce their impact on the science data and subsequently increase the accuracy of the gravity field solutions. Moreover, understanding the complexity of the onboard system is essential not only for increasing the accuracy of the GRACE data but also for the development of the future gravity field satellite missions.     

Numerical simulation of broken pin effects on the flow field and cooling performance of a double-wall cooling configuration

In this paper, the flow characteristics of the double wall structure are presented and the effect of the broken pin size on the cooling performance and flow field of the double wall configuration is investigated. A periodic plate model with seven units is adopted, and there are an impingement hole and a film hole in each unit. Under five blowing ratios, six different sizes of the broken pin are compared, and the double wall configuration without broken pins is taken as the baseline. The results show that if the broken pins height is too small, the cooling effectiveness usually cannot be improved. With the presence of broken pins with a height of more than 0.4, the effectiveness is improved due to the enhancement of reattachment and recirculation of coolant. With the increase of the broken pin height, the cooling effectiveness increases. However, the increase of the diameter does not always improve the cooling performance, since the limiting effect of the wall jet. In this study, Case 6 with the largest broken pin always has the best cooling performance, but also the largest flow resistance. In Case 6 temperature is reduced by almost 15 K compared to the baseline, and more areas have relatively higher cooling effectiveness.     

基于并行运算体系结构的星敏感器图像处理算法

采用FPGA构建星敏感器图像处理并行计算体系结构。星敏感器图像处理算法由高通滤波、星点提取和星点排序3个模块组成。高通滤波模块基于图像局部加窗计算阈值的方法,星点提取模块采用逐行扫描的计算方法,星点排序模块采用基数排序的计算方法。星敏感器图像处理算法基于四级流水并行计算体系结构,显著提高了星敏感器图像处理的效率和算法的可靠性。
     

等离子体中稳恒流形成电双层的机制

在考虑稳恒流产生磁场的基础上,通过求解双时标,双流体方程组,从理论上对电双层形成的机制进行了研究,解释了实验室中产生电双层现象所必须引入的条件──必须有带电粒子流的注入．     

星敏感器图像处理系统的并行流水线操作研究

随着天文导航和航天测控领域的要求不断提高,对星敏感器的动态性能提出了越来越高的要求。本文详细分析了星敏感器CCD处理模块输出信号的时序关系,在此基础上提出了CCD和DSP并行流水线的处理机制以提高星图处理的效率,并利用CPLD和DSP的HOLD方式实现了CCD和DSP的并行流水线操作。通过星光模拟器的静态测试表明:利用该处理机制能实现每秒10帧的处理速度。只要合理地安排好行场有效期和消隐期的时间,会进一步提高姿态捕获的速度。     

一种新式宽带宽方向图圆极化双环天线

提出了一种结构新颖的双环天线,该天线具有结构简单、宽带、宽波束、圆极化等诸多优点,通过实验测试方法验证了设计的有效性。同时提出了通过附加反射板的方法提高了该天线的低仰角增益,并对天线的输入阻抗和圆极化轴比有一定的改善作用。     

一种基于三正交主轴平面的快速星图模拟方法

为在地面上进行星图模拟以测试星图识别算法和星敏感器性能, 提出了一种新的快速星图模拟方法. 该方法利用截面圆和固定区域的性质, 将单位天球按照三个正交主轴平面进行等分, 根据赤纬值求解恒星矢量与主轴平面夹角来确定选星条件, 进而根据坐标变换原理进行星图模拟. 为验证所提方法与现有方法相比的优势, 进行了大量的仿真实验. 实验结果表明, 与现有星图模拟方法相比, 本文方法在保证星图模拟精度的条件下, 选星速度提高了3倍以上.      

基于双判定准则的航空发动机叶片缺陷孔洞的边界提取

航空发动机叶片缺陷孔洞的几何形状复杂、位置分布散乱且曲率变化明显,使用单一判定准则难以完整地提取其边界特征点.为实现叶片缺陷孔洞边界的精准提取和孔洞边界线的平滑拟合,提出了一种基于双判定准则的航空发动机叶片缺陷孔洞边界特征点的提取算法.该算法采用K–Dimension tree(K–D树)建立点云的空间拓扑结构,以采样...