天问一号探测器高动态着陆惯导系统设计与试验

考虑到火星探测任务着陆过程动态变化大,稀薄大气环境下开伞会对探测器产生剧烈晃动,为此天问一号探测器研制了一套高动态着陆惯导系统,从硬件产品、使用时序到导航算法方面均进行了针对性设计,以适应着陆过程中的高动态环境.此外,为验证天问一号探测器高动态着陆惯导系统的性能,设计了模拟火星开伞工况的火箭弹高空开伞试验,结果表明该高...     

基于CCSDS空间数据链路安全协议的星载遥控认证保护

在国际空间数据系统咨询委员会(CCSDS)规定的空间遥控系统数据传输体制下,对星载遥控认证保护进行了研究。选择了遥控数据认证保护层次,并设计了认证保护数据范围。针对上行遥控的认证保护机制与国际空间数据系统咨询委员会的空间遥控链路命令操作过程(COP-1)之间存在的"闭锁"风险,设计了重传请求保护机制。基于空间数据链路安全(SDLS)协议体制,提出了一种遥控认证帧结构模型。在该模型中,通过插入随机序列码段,使相同指令/数据帧经认证算法计算后,其结果的非线性度扩大;通过插入毫秒级精度的时间序列码段,抵御重放攻击,并极好地适应不同地面控制中心对航天器的并行控制。提出一种针对遥控认证保护的,涉及"常态"和"应急态"的安全关联(SA)周期管理的方法、密钥生存周期管理的方法,有效实现各虚拟信道的独立保护及密钥的科学管理。同时,提出一种开展星载遥控认证保护业务的算法设计方法。     

基于S1,S2流面理论的液体火箭发动机涡轮内部流场计算

应用S1,S2流面理论对某大型液氢/液氧火箭发动机涡轮泵的两级轴流式涡轮内部跨声速流场进行计算和分析。流面的求解采用流线曲率法。将混合平面法的思想用于流线曲率法的求解过程中,对动、静叶排之间的相互干扰进行处理,将复杂的非定常问题简化为定常问题,从而简化计算。粘性的影响通过几种损失系数进行修正。计算结果较好地描述了涡轮内部的流动情况,为进一步完善涡轮设计、提高涡轮性能提供了理论依据。     

中俄联合火星电离层星-星掩星探测

中俄联合火星星-星掩星探测是人类首次在火星空间环境进行此类的联合试验。用于探测火星电离层的星-星掩星技术较以前星地间的探测技术相比,有可接收高信噪比信号,反演精度高,可探测火星上太阳天顶角大于43°,或者小于138°的区域电离层等优点。本文介绍了中俄联合火星星-星掩星探测方案、基本原理,给出了主要技术指标、地面模拟测试结果。     

Variable Structure Control of Catastrophic Course in Airdropping Heavy Cargo

The mathematical model of a transport aircraft would be subjected to a sudden change when heavy cargo is dropped off in airdropping, which exerts serious influences upon the safety of the aircraft. A variable structure controller is specially designed for handling the airdrop process. The nonlinear system is linearized by input-output feedback linearization using differential geometry theories. On this basis, an inner loop system for velocity and attitude tracking control is designed by using the exponentially approaching rule of the variable structure theory. The whole flight control system is integrated with the outer loop flight altitude control. Digital simulation evidences the applicability of the system to potentially catastrophic course in airdropping heavy cargo and provides robustness against system parameter perturbation.     

基于FGN输入流的G/D/1排队模拟

传统的排队理论不适于分析高速网络表现出的自相似流量.通过实验仿真,主要考察平均等待时间和在队列分别为无限和有限情形下的队列尾部特征等参数,并对以FGN为输入流的G/D/1排队模型作了定性分析.结果表明在输入流的强度和方差基本相等且系统利用律大于某一阈值的情况下,队列平均等待时间随Hurst参数增大而显著增长.同时指出在相同的条件下考察队列尾部特征,具有有限队列长度的G/D/1排队模拟结果要远优于无限队列长度下的理论分析结果.      

任务教学法在Protel 99 se课程教学中的应用

任务教学法是一种以学生为中心,以任务为驱动的教学方法,它适用于实践性很强的prote199se课程.在一个个任务完成后,激发了学生自主学习的积极性,使学生在实践中学会了各种命令的使用,掌握了技巧,从而可以取得满意的教学效果.     

Orbital phase spectroscopy of four high mass X-ray binary pulsars to study the stellar wind of the companion

Our work focuses on a comprehensive orbital phase-dependent spectroscopy of the four High Mass X-ray Binary Pulsars (HMXBPs) 4U 1538-52, GX 301-2, OAO 1657-415 and Vela X-1. We hereby report the measurements of the variation of the absorption column density and iron-line flux along with other spectral parameters over the binary orbit for the above-mentioned HMXBPs in elliptical orbits, as observed with the Rossi X-ray Timing Explorer (RXTE) and the BeppoSAX satellites. A spherically symmetric wind profile was used as a model to compare the observed column density variations. Out of the four pulsars, only in 4U 1538-52, we find the model having a reasonable corroboration with the observations, whereas in the remaining three the stellar wind seems to be clumpy and a smooth symmetric stellar wind model appears to be quite inadequate in explaining the data. Moreover, in GX 301-2, neither the presence of a disk nor a gas stream from the companion was validated. Furthermore, the spectral results obtained in the case of OAO 1657-415 and Vela X-1 were more or less similar to that of GX 301-2.     

The effect of neglecting VLBI reference station clock offsets on UT1 estimates

Very Long Baseline Interferometry (VLBI) allows to monitor universal time (UT1) by conducting regular international experiments. Such dedicated observation networks are equipped with different hardware components, which require different processing strategies when the data are correlated. As the timing units at each stations are usually offset with respect to universal time (UTC) this effect should be considered during correlation processing. Thus, it is investigated how neglecting of these offsets theoretically impacts the estimation of UT1. Three different strategies for the proper handling of the timing offset will be discussed and their advantages/drawbacks will be pointed out. Moreover, it is studied how neglecting of these timing offsets affects UT1 time-series and how such a missing correction can be applied a posteriori. Although the discussed effect is for most of the UT1 experiments smaller than the formal error of the estimates, it is important to consider station clock offsets properly in next-generation VLBI systems, which are expected to improve accuracy of results by about one order of magnitude.     

Introduction to the Payloads and the Initial Observation Results of Chang＇E-1

Chang'E-1,the orbiter circling the moon 200km above the moon surface,is the first Chinese Lunar exploration satellite.The satellite was successfully launched on 24th October 2007.There are 8 kinds of scientific payloads onboard,including the stereo camera,the laser altimeter,the Sagnac-based interferometer image spectrometer,the Gamma ray spectrometer,the X-ray spectrom-eter,the microwave radiometer,the high energy particle detector,the solar wind plasma detector and a supporting payload data management system.Chang'E-1 opened her eyes to look at the moon and took the first batch of lunar pictures after her stereo camera was switched on in 20th November 2007.Henceforth all the instruments are successfully switched on one by one.After a period of parameter adjustment and initial check out,all scientific instruments are now in their normal operating phase.In this paper,the payloads and the initial observation results are introduced.