Usage of pre-flight data in short rendezvous mission of Soyuz-TMA spacecrafts

The paper describes the reduction of the vehicle autonomous flight duration before docking to the ISS. The Russian Soyuz-TMA spacecraft dock to the ISS two days after launch. Due to the limited volume inside Soyuz-TMA the reduction of time until docking to the ISS is very important, since the long stay of the cosmonauts in the limited volume adds to the strain of the space flight. In the previous papers of the authors it was shown that the existing capabilities of Soyuz-TMA, the ISS and the ground control loop make it possible to transfer to the five-orbit rendezvous profile. However, the analysis of the cosmonauts' schedule on the launch day shows that its duration is at the allowable limit and that is why it is necessary to find a way to further reduce the flight duration of Soyuz-TMA before docking to less than five orbits. In a traditional rendezvous profile, the calculation of rendezvous burns begins only after determination of the actual vehicle insertion orbit. The paper describes an approach in which the first two rendezvous burns are performed as soon as the spacecraft reaches the reference orbit and the values of the burns are calculated prior to the launch based on the pre-flight data for the nominal insertion. This approach decreases the duration of the rendezvous by one orbit. The demonstration flight of a Progress vehicle using the proposed profile was implemented on August 1, 2012 and completely confirmed the correctness of the imbedded principles. The paper considers the possible improvements of the proposed approach and recovery from the contingencies.     

对信息检索系统应用技术的数学表示模型的分析

页面表示、用户兴趣模型、页面链接排序是信息检索系统中的关键技术,分析相应的数学模型,并例举在一个智能搜索引擎中的应用,通过动态的更新用户兴趣模型和由此而引起的WEB页面更新,有效地适应用户兴趣的变化。     

脉冲星导航试验卫星科学观测数据分析

脉冲星导航试验卫星是我国发射的一颗专用试验卫星.经过4个多月的在轨观测,该卫星已成功获取了大量观测数据.介绍利用该卫星搭载的掠入射聚焦型X射线探测器在近4个月中对PSR B0531+21获得的观测数据第一批处理结果.本文详细阐述掠入射聚焦型X射线探测器的观测模式,给出脉冲星观测数据的处理方法以及脉冲星参数的拟合过程,利用基于第一手观测数据的脉冲星精化参数验证掠入射聚焦型探测器在轨工作性能,得以回答使用国产X射线探测器是否能够“看得见”脉冲星问题.     

导弹助推器分离过程数值模拟研究

应用了结构网格中的Chimera重叠网格技术和Favre平均三维N-S方程以获得流场解.采用k-ε湍流模型模拟气体的湍流粘性影响,计算中分别考虑空气和两种火箭发动机喷流等三种不同流动介质,采用时间相关边界模拟发动机拖尾段的非定常流动,最终求解带约束的六自由度弹道方程模拟了导弹助推器的分离脱落过程.并对发动机喷流对助推器分离的影响开展研究.所做工作可对于精确确定火箭助推器分离轨迹及姿态提供方法参考.      

宽带相控阵雷达各模块幅相失真对成像的影响

宽带LFM信号作为一种广泛应用于宽带相控阵雷达系统中的信号,在实际应用中一般可采用Stretch处理的方法,实现高距离分辨成像,并大大减少数据采集难度.但它需要很大的瞬时带宽,传统上认为当瞬时带宽较大时,系统的幅相频率特性难以满足要求.通过对实测数据的分析,发现当有源相控阵模块较多时,由于模块之间幅相失真的综合作用,虽然单个模块存在较大的幅相误差,但最终雷达成像性能仍满足设计要求.     

Photospheric flows in the active regions (asymmetric and localized Doppler velocities)

We observed 10 active regions through their disk passage during June 25–August 25, 1988, with the Tower Vector Magnetograph (TVM) of Marshall Space Flight Center. The TVM was used in scanning mode to measure the photospheric Doppler velocities with the Line-Center-Magnetogram (LCM) technique in the spectral line of FeI 5250.2 Å. In this paper we present the result of a subset of observations obtained while the active regions were situated away from the solar limb. A wide range of magnetic complexity and associated chromospheric activity characterized these active regions. It was found that the value of zero-crossing wavelength of the integrated Stokes-V profile of two opposite magnetic polarities were different, corresponding to Doppler velocities ranging from ∼100 m s⁻¹ to ∼1475 m s⁻¹. The measurements of relative velocities between different locations, connected by magnetic flux tubes as inferred from YOHKOH soft X-ray and TRACE 171 Å Fe IX images, showed widely different values of dominant localized flows. The region of parasite polarity, which showed recurrent chromospheric activity, was blue shifted with respect to the main “magnetic element” of the same polarity. Some of them were also the sites of sheared magnetic field configuration. The magnitude of the relative velocity between the leading and following polarity is more for the active regions of higher “field asymmetry”.     

多普勒测风激光雷达风廓线探测精度对比分析

在晴空干洁的大气条件下,多普勒测风激光雷达能够以较高的时间、空间分辨率,获得大气三维风场信息。为验证北京遥测技术研究所研制的WINDLE LIDAR型多普勒测风激光雷达探测的准确性,2020年4月~5月,用该雷达在北京市南郊观象台和L波段探空雷达进行同时同址对比观测。2022年6月~7月,用该雷达与北京遥测技术研究所的WINDLE U7相干测风激光雷达进行同时同址对比观测。通过对数据进行相关性分析,得到比对结果如下：1）垂直探测距离大于5 km,最大探测高度可达8.5 km;2）与L波段探空雷达对比,风速和风向数据拟合总相关系数分别为0.990和0.998。总体风速和风向的系统偏差、标准偏差分别为0.114 m/s和3.078°、0.489 m/s和3.969°,二者具有较好的一致性;3）与WINDLE U7雷达对比,风速和风向数据拟合总相关系数分别为0.999和0.999。总体风速和风向的系统偏差和标准偏差分别为0.209 m/s和1.077°、0.255 m/s和1.220°,可以看出该雷达系统的优越性。     

基于齿廓修形的锥齿轮再制造技术

锥齿轮是航空发动机传动系统中的重要组成部分,在使用过程中容易产生齿面磨损、齿面点蚀、齿面剥落、齿面胶合等故障。文中分析了锥齿轮故障原因及再制造可行性,构建了锥齿轮的再制造判别标准,制订了以齿廓修形技术为核心的锥齿轮再制造工艺方法。通过检测渗碳层深度、硬度,试验验证,齿轮装配检查,台架试车考核表明：再制造的锥齿轮渗碳层深度、显微硬度符合设计要求,齿轮啮合间隙、着色印痕以及试车后齿面金属印痕均符合技术要求,装机试用的锥齿轮传动平稳,啮合性能好,产生的振动和噪声小。再制造成本仅为新品的11.3%,节能效果为86%,节材78%,取得了显著的经济和社会效益,具有广阔的应用前景。     

评定线轮廓度误差的通用数学模型

建立了用最小二乘法评定平面曲线轮廓度的通用数学模型。运用该模型可对任意平面曲线的轮廓度进行评定，从而将直线度、圆度、椭圆度以及任何线轮廓度的评定归结在统一的模式中。由于所建立的模型直观、明了，很容易在计算机上实现，因而可在生产实际中普遍推广应用。举例说明了线轮廓度误差可分离成形状误差、参数误差和位姿误差，给出了分离公式和误差补偿原则。     

基于目标一维距离像的雷达目标识别方法

讨论了马氏距离的性质,利用目标的一维距离像,提出了一种雷达目标识别方法.对雷达回波进行快速傅立叶变换,得到目标的一维距离像,计算其马氏距离,得到目标的稳定特征向量,根据相关算法进行目标识别.三种不同类型飞机回波的实测数据的识别结果,表明该方法是切实可行的.