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1.
针对高超声速变形飞行器再入制导问题,提出了一种采用伸缩式机翼的高超声速变形飞行器外形方案,建立了含有展长变形量的气动模型和动力学模型。将该变形飞行器的展长变形量扩展为控制变量,分析了倾侧角、展长变形量和终端航程、高度之间的关系。在此基础上,利用倾侧角和展长变形量在线预测剩余航程和终端高度,通过数值方法校正2个控制量以满足航程约束和高度约束,通过航向角走廊确定倾侧角符号。仿真结果表明:该变形飞行器再入制导方法制导精度高,相比于传统固定外形飞行器终端约束能力更强、轨迹更加平滑,且在扰动条件下具有一定鲁棒性。 相似文献
2.
Yongliao Zou Yan Zhu Yunfei Bai Lianguo Wang Yingzhuo Jia Weihua Shen Yu Fan Yang Liu Chi Wang Aibing Zhang Guobin Yu Jihong Dong Rong Shu Zhiping He Tielong Zhang Aimin Du Mingyi Fan Jianfeng Yang Yongqing Peng 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(2):812-823
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. 相似文献
3.
针对空天往返飞行器的返回滑翔段在线制导问题,设计了一种新的滑翔段飞行剖面,实现了滑翔段终端交班高度、位置和倾角约束的自动满足,减少了在线制导算法中需处理的约束数量。推导了滑翔段运动状态、过程约束和性能指标的解析表达式,获得了剩余航程和终端速度间的函数关系。在此基础上,提出了一种双层在线制导方法:内层解析重构飞行剖面,同时通过解析确定路径点来改变剩余航程的变化率,进而对终端交班速度进行控制;外层借助解析表达式,使用粒子群优化算法(PSO)和改进共轭梯度法(CGM)优化飞行剖面,从而满足过程约束和指标要求。最后通过数学仿真验证了方法的正确性。 相似文献
4.
针对多臂空间机器人自主目标抓捕任务,首先建立多臂空间机器人的运动模型和其与目标的相对运动模型,采用Kane方法建立多臂空间机器人的动力学模型;其次,研究基于视觉伺服的机械臂在线轨迹规划算法,并引入零反作用机动,消除机械臂运动对平台姿态的扰动;再次,在不使用零反作用机动功能时,分别使用基于角动量前馈补偿的协调控制算法和逆动力学方法设计了协调控制器,在机械臂运动时保持平台姿态和相对目标的位置。最后,开发了基于Matlab的仿真软件MASS(多臂空间机器人仿真),仿真结果校验了上述方法的有效性。 相似文献
5.
Xingyuan Yan Guanwen Huang Qin Zhang Chenchen Liu Le Wang Zhiwei Qin 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(3):1270-1279
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. 相似文献
6.
7.
针对未来低运行成本、可直接水平起降、重复使用的大型天地往返运输系统平台飞行器研制所需重点解决的全速域气动力性能需求与气动热防护匹配等难题,分析了典型航天飞机方案所存在的能量运行缺陷等主要问题及可能的改善方案。基于放宽气动热防护设计、涡轮/冲压/火箭发动机三动力组合、嵌套式旋转机翼全速域变体、在爬升阶段将飞行动能转化为高度势能以及再入阶段“跳跃式”盘旋减速飞行轨迹控制等设计思想,从能量损失速率控制和回收利用等角度出发,开展了一种新型大型天地往返运输系统平台气动布局概念设计研究。全速域气动力/热性能工程估算以及内/外流整体气动效能初步分析结果表明,该方案可有效满足整个飞行包线内的升重平衡需求,相比航天飞机方案具有显著的整体气动效能优势,值得进一步开展深入研究。 相似文献
8.
Jia Luo Fangfang Sun Xiaohua Xu Han Wang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(1):327-336
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. 相似文献
9.
Mukul Kumar Wang Chi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(1):640-652
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. 相似文献
10.