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1.
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   
2.
铌掺杂ITO镀膜玻璃电磁散射特性试验   总被引:1,自引:1,他引:0       下载免费PDF全文
座舱玻璃镀膜是实现飞行器隐身技术的重要途径之一。利用雷达散射截面(RCS)均值增益研究铌掺杂ITO镀膜玻璃隐身性能;针对不同方块电阻的铌掺杂ITO镀膜玻璃,进行系列化RCS暗室测试,分析不同入射频率、极化方式的电磁散射特性。结果表明:方块电阻增大时电磁散射减弱,合适的方块电阻(小于40Ω/m~2)有利于实现座舱外形隐身,散射特性与金属接近,频率较高时,镜面散射波峰较窄。  相似文献   
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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   
4.
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   
5.
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   
6.
郝旺  王占学  张晓博  周莉  王为丽 《推进技术》2021,42(9):2011-2021
为了降低传统迭代算法在求解变循环发动机非线性模型时对初值的依赖性,将模型的求解问题转换为求最小值的优化问题,引入差分进化算法进行模型的求解,并提出一种自适应差分进化算法(ADE)。ADE借助轮盘赌选择法,利用种群的进化经验可以自适应的选择最适合当前种群的差分策略与算法控制参数。针对变循环发动机四个典型工作点的模型求解问题,研究了标准差分进化算法(SDE)的控制参数对其性能的影响,获取了SDE在求解四个典型工作点时的最优控制参数组合,对比分析了ADE与SDE的性能差异,最后研究了种群规模对ADE性能的影响。结果表明:SDE在求解发动机模型时具有较好的鲁棒性,在求解不同工作点时算法的最优控制参数并不完全相同;相比于使用最优控制参数的SDE,ADE可以在不影响算法鲁棒性的情况下提升效率50%以上;减少ADE的种群规模会在提升算法效率的同时破坏鲁棒性。  相似文献   
7.
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.  相似文献   
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