高压捕获翼构型的跨流域气动特性

高压捕获翼(HCW)构型是一种满足高速飞行器高容积、高升力、高升阻比的设计需求的新型气动布局.最近研究表明,HCW构型能够提高飞行器在连续流区的升力和升阻比,缓解飞行器设计中高容积率与高升阻比间的矛盾.为探究该气动布局在过渡流域(70～100 km)的气动特性,以一种楔—平板组合的高压捕获翼原理性构型作为模型,采用直接模拟Monte Carlo(DSMC)方法,详细分析了该模型在典型高超声速条件(马赫数20)下的流场结构和壁面气动力/热分布.结果表明,随着飞行高度增加,稀薄效应增强,机体压缩产生的激波厚度增加,激波边缘逐渐模糊,机体与捕获翼之间的开放通道内出现压力干扰.同时,高压捕获翼表面的摩擦系数迅速上升,气动摩擦成为制约捕获翼构型升阻比的重要因素.针对这一问题,分析了捕获翼材料表面的适应系数对飞行器的气动力/热的影响,结果表明,降低适应系数可以显著减小壁面摩擦和热流量,可通过选用适应系数较小的表面材料进一步提高该类飞行器气动性能.     

磁浮飞行风洞试验技术及应用需求分析

随着高速、超高速轨道交通的快速发展,需要发展新型的风洞设备,实现风洞性能和试验能力的突破.磁浮飞行风洞是利用真空管道列车概念结合动模型试验技术提出的一种新概念风洞设备,可以构建出更加接近真实状态的测试环境.本文从磁浮飞行风洞基本概念、国内外研究现状及发展趋势、试验技术、应用需求等几个方面开展论述.首先论述了国内外传统风洞和动模型设备的现状及发展趋势,指出了发展磁浮飞行风洞的必要性;其次,重点对磁浮飞行风洞需要发展的试验技术进行了分析;最后,对磁浮飞行风洞在超高速轨道交通及其他领域的应用需求进行了展望.     

Scientific objectives and payloads of Tianwen-1, China’s first Mars exploration mission

This paper describes the scientific objectives and payloads of Tianwen-1, China’s first exploration mission to Mars. An orbiter, carrying a lander and a rover, lifted-off in July 2020 for a journey to Mars where it should arrive in February 2021. A suite of 13 scientific payloads, for in-situ and remote sensing, autonomously commanded by integrated payload controllers and mounted on the orbiter and the rover will study the magnetosphere and ionosphere of Mars and the relation with the solar wind, the atmosphere, surface and subsurface of the planet, looking at the topography, composition and structure and in particular for subsurface ice. The mission will also investigate Mars climate history. It is expected that Tianwen-1 will contribute significantly to advance our scientific knowledge of Mars.     

Early analysis of precise orbit and clock offset determination for the satellites of the global BeiDou-3 system

Eight new-generation BeiDou satellites (BeiDou-3) have been launched into Medium Earth Orbit (MEO), allowing for global coverage since March 2018, and they are equipped with new hydrogen atomic clocks and updated rubidium clocks. Firstly, we analyzed the signals for the carrier-to-noise-density ratio (C/N0) and pseudorange multipath (MP) by using international GNSS (Global Navigation Satellite System) Monitoring and Assessment System (iGMAS) station data, and found that B1C has a lower C/N0, and B2a has the same level of C/N0 as the B1I and B3I signals. For pseudorange multipath, compared with the BeiDou-2 satellites, the obvious systematic variation of MP scatters related to the elevation angle is greatly improved for the BeiDou-3 and BeiDou-3e satellites signals. For the signals of the BeiDou-3 satellites, the order of the Root Mean Square (RMS) values of multipath and noise is B3I?<?B1I?<?B2a?<?B1C. Then, the comparison of the precise orbit determination and clock offset determination for the BeiDou-2, BeiDou-3, and BeiDou-3 experimental (BeiDou-3e) satellites was done by using 10 stations from iGMAS. The 3D precision of the 24?h orbit overlap is 24.55, 25.61, and 23.35?cm for the BeiDou-3, BeiDou-3e, and BeiDou-2 satellites, respectively. BeiDou-3 satellite has a comparable precision to that of the BeiDou-2 satellite. For the precision of clock offset estimation, the Standard Deviation (STD) of the BeiDou-3 MEO satellite is 0.350?ns, which is an improvement of 0.042?ns over that of the BeiDou-2 MEO satellite. The stabilities of the BeiDou-3 and BeiDou-3e onboard clocks are better than those of BeiDou-2 by factors of 2.84 and 1.61 at an averaging time of 1000 and 10,000?s, respectively.     

Ionospheric F2-Layer critical frequency retrieved from COSMIC radio occultation: A statistical comparison with measurements from a meridional ionosonde chain over Southeast Asia

In this paper, we compared the F2-Layer critical frequency (foF2) derived from FORMOSAT-3/COSMIC radio occultation (RO) and ionosondes at Chiang Mai, Chumphon and Kototabang during the years 2008–2015 to evaluate the performance of COSMIC RO over Southeast Asia region. The results show that the time development of foF2 values derived from COSMIC RO generally agrees well with those from ionosonde measurements. However, the differences between the foF2 derived from COSMIC RO and that derived from ionosonde observations display latitudinal dependence. COSMIC RO tends to underestimate foF2 at Chiang Mai and Kototabang, which is near to the north EIA crest and the south one, respectively, while a little overestimate foF2 at Chumphon, which is close to the geomagnetic equator. COSMIC RO agrees best with ionosonde at Chumphon and worst at Chiang Mai. At each ionosonde station, the quality of COSMIC RO data degrades with the increase of solar activity. In addition, at the station Chiang Mai and Kototabang, COSMIC RO performs better in summer than in equinox and winter. Furthermore, the differences in foF2 derived from COSMIC RO and that from ionosonde measurements vary with local time, i.e., the differences in foF2 are generally smaller at night and larger in noontime when equatorial ionization anomaly (EIA) is well developed.     

Alfvén gravity waves in viscous solar plasma: Effect of the background flow

We study the Propagation and damping properties of Alfvén gravity waves in the presence of the vertical magnetic field in the viscous solar plasma under influence of the background flow by deriving a fourth order dispersion relation in terms of the Doppler shifted frequency. We derive the dispersion relation under WKB and Boussinesq approximation. We study the damping of Alfvén gravity waves for the wave frequencies less than and greater than the Brunt-Väisälä frequency. We find that the Brunt-Väisälä frequency divides the frequency ranges where the weakly or strongly damped oscillations occur. The background flow exhibits a strong effect on weakly damped oscillations and a weak effect on the strongly damped oscillations. We also notice that the damping of both the strong and weakly damped oscillations depend on the Brunt-Väisälä frequency and wave number. The effect of the background flow is also being governed by the Brunt-Väisälä frequency and wave number. We also study the properties of gravity wave mode after filtering the Alfvén wave mode by minimizing the magnetic field and noticed that the background flow shows a very strong effect on the gravity wave mode.     

面向下一代运载火箭的综合电子系统集成技术

介绍了面向下一代运载火箭分布式模块化电子系统(DIMA)的集成技术及系统架构。针对下一代运载火箭复杂电子系统的特点，按照系统集成的路线，对系统设计目标、系统功能需求分析、系统抽象机制、系统综合技术等多方面进行论述。首先，根据电气系统功能获得系统需求，采用功能抽象和层次抽象定义系统抽象模型，提取出高内聚低耦合的原子功能模块，并对模块的属性、交换关系、时序约束关系等进行定义；然后采用可视化表征方法对系统进行深入分析，利用系统综合技术实现了从系统功能到硬件资源的映射，从而给出了集成控制单元和模块的种类；随后采用分时分区的设计理念对系统节点分区划分方案及容错架构进行了定义，并对分区操作系统的调度模型和交换式的数据交互网络进行了论述，最终给出了系统软硬件架构。     

无人集群系统时变编队H∞控制

针对有向通信拓扑网络下具有通信时滞与外部干扰的无人集群系统（AUSS）时变编队H_∞控制问题进行了研究。首先，基于AUSS期望编队构型信息、无人机（UAV）实时状态信息以及通信UAV之间带通信时滞的状态误差信息提出了AUSS的编队控制方法，通过变量替换将AUSS的编队控制问题转换成低维闭环系统的渐近稳定问题，并以线性矩阵不等式（LMI）形式给出了系统稳定的充分条件与最大允许通信时滞的计算公式。其次，通过构造Lyapunov-Krasovskii（L-K）泛函，证明了存在通信时滞与外部干扰条件下AUSS能够实现时变编队。最后，通过数值仿真验证所设计方法的准确性与有效性。      

基于飞行数据分析的发动机故障诊断系统研究

依据现有的发动机故障诊断方法,研究发动机故障诊断系统,通过对飞行数据中反映发动机性能指标的关键参数数据进行分析,说明系统对航空发动机故障诊断的可行性和必要性,研究结果对于提高发动机维护的快速性和准确性具有重要意义.