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811.
在空间柔性机械臂的动力学与控制问题中,逆动力学求解常要求有较高的计算速度.当柔性多体系统受到高频激励时,必须考虑高阶模态才能保证足够的计算精度,但同时提高了计算自由度数,降低了计算速度.为了提高此类问题的计算效率,本文将模态自适应策略应用于旋转柔性臂逆动力学建模,计算了高频激励下产生期望旋转运动的柔性臂关节驱动力矩,验证了该方法的有效性,并研究了重力对计算结果的影响. 相似文献
812.
As scientific experiment payloads, microgravity experiments of fluid physics, life science,combustion science, physics and accelerator measurement were conducted on board the Chinese recoverable satellite SJ-8 during 18-day orbital flight. The experimental payloads and an experiment support system constituted the microgravity experiment system of the flight mission. This article has presented the briefs of the scientific achievements of these space experiments, the composition and performance of the Microgravity Experimental System (MES) and the general picture of the overall flight mission, respectively. 相似文献
813.
Phillip C. Chamberlin Thomas N. WoodsFrancis G. Eparvier 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
The solar photon output from the Sun, which was once thought to be constant, varies considerably over time scales from seconds during solar flares to years due to the solar cycle. This is especially true in the wavelengths shorter than 190 nm. These variations cause significant deviations in the Earth and space environment on similar time scales, which then affects many things including satellite drag, radio communications, atmospheric densities and composition of particular atoms, molecules, and ions of Earth and other planets, as well as the accuracy in the Global Positioning System (GPS). The Flare Irradiance Spectral Model (FISM) is an empirical model that estimates the solar irradiance at wavelengths from 0.1 to 190 nm at 1 nm resolution with a time cadence of 60 s. This is a high enough temporal resolution to model variations due to solar flares, for which few accurate measurements at these wavelengths exist. This model also captures variations on the longer time scales of solar rotation (days) and solar cycle (years). Daily average proxies used are the 0–4 nm irradiance, the Mg II c/w, F10.7, as well as the 1 nm bins centered at 30.5 nm, 121.5 (Lyman Alpha), and 36.5 nm. The GOES 0.1–0.8 nm irradiance is used as the flare proxy. The FISM algorithms are given, and results and comparisons are shown that demonstrate the FISM estimations agree within the stated uncertainties to the various measurements of the solar Vacuum Ultraviolet (VUV) irradiance. 相似文献
814.
N.G. Ptitsyna V.V. Kasinskii G. Villoresi N.N. Lyahov L.I. Dorman N. Iucci 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,42(9):1510-1514
Intense geomagnetically induced currents (GIC) can hamper rail traffic by disturbing signaling and train control systems. GIC threats have been a concern for technological systems at high-latitude locations due to geomagnetic disturbances driven by substorm expansion electrojet or convection electrojet intensifications. However, other geomagnetic storm processes such as storm sudden commencement (SSC) and geomagnetic pulsations can also cause GIC concerns for technological systems. We present in this paper the first evidence based on statistical data for links between geomagnetic disturbances and faulty operations (anomalies) in the functioning of railway automatics and telemetry. We analyze anomalies of automatic signaling and train control equipment which occurred in 2004 on the East-Siberian Railway (corrected geomagnetic latitude m = 46–51°N and longitude λm = 168–187°E). Our results reveal a seasonal effect in the number of anomalies per train similar to the one observed in geomagnetic activity (Kp, Ap, Dst indices). We also found an increase by a factor of 3 in the total duration of daily anomalies during intense geomagnetic storms (local geomagnetic index specific to Siberian Observatory Amax > 30), with a significant correlation between the daily sum of durations of anomalies with geomagnetic activity. Special attention was paid to failures not related to recognized technical malfunctions. We found that the probability of these failures occurring in geomagnetically disturbed periods was 5–7 times higher than the average anomaly occurrence. 相似文献
815.
S. Torii K. Yoshida K. Kasahara T. Tamura J. Chang for the CALET Collaboration 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(12):2032-2036
The CALorimetric Electron Telescope, CALET, mission is proposed for the observation of high-energy electrons and gamma-rays at the Exposed Facility of the Japanese Experiment Module on the International Space Station. The CALET has a capability to observe the electrons (without separation between e+ and e−) in 1 GeV–10 TeV and the gamma-rays in 20 MeV–several TeV with a high-energy resolution of 2% at 100 GeV, a good angular resolution of 0.06 degree at 100 GeV, and a high proton-rejection power of nearly 106. The CALET has a geometrical factor of 1 m2sr, and the observation period is expected for more than three years. The very precise measurement of electrons enables us to detect a distinctive feature in the energy spectrum caused from WIMP dark matter in the Galactic halo. The excellent energy resolution of CALET, which is much better than GLAST or air Cherenkov telescopes over 10 GeV, enables us to detect gamma-ray lines in the sub-TeV region from WIMP dark matter annihilations. The CALET has, therefore, a unique capability to search for WIMP dark matter by the hybrid observations of electrons and gamma-rays. 相似文献
816.
空间碎片超高速撞击动力学建模与数值仿真技术 总被引:12,自引:0,他引:12
阐明了空间碎片超高速撞击数值仿真技术研究的目的、意义和国内外发展状况 ;重点论述了空间碎片超高速撞击数值仿真技术的主要研究内容、技术指标和具体实施途径 ,从而为研究的深入开展提供了技术依据和指导原则 相似文献
817.
王希季 《中国空间科学技术》2002,22(5):1-8
在“神舟号”载人飞船工程实现了中国人往返于天地间的目的之后 ,中国应审慎地选择发展载人航天的目标。文章从中国社会对载人航天的需求出发 ,讨论了以开发利用空间微重力物质环境为目标的空间站和以发展天基航天为目标的天基航天站的外部工程系统的环境条件 ,认为中国在运载火箭、发射和回收场、测控站网方面已有较好基础 ,基本具备条件 ,运人运输器已有“神舟号”载人飞船 ,运物运输器的研制也不困难 ,但在为保障航天员在空间生活、工作的航天员系统方面和为实现载人航天工程功能和显现价值的有效载荷系统方面欠缺较多 ,需要一个研究、试验、培训和开发、演示的发展阶段 相似文献
818.
分析对比了空间目标与可控飞行器轨道确定的不同,论述了太阳翼定向模式的不同对轨道运动特性的影响。通过地面站的测距与测角数据,推算出测量数据的地心距频谱。假定一种太阳翼定向模式,利用测量数据进行轨道确定,利用定轨数据计算地心距频谱并与测量数据的频谱比对,由此可确定太阳翼定向模式。利用数值仿真对近地太阳同步轨道和地球静止轨道两种情况进行了验证,仿真结果表明该思路和方法是有效的。 相似文献
819.
820.