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781.
782.
为考察在大气层内拦截弹上应用直接侧向力与气动力复合控制同应用纯气动力控制的本质区别,依据连续系统跟踪性能极限的研究成果,提出以复合控制对象的非最小相位零点作为描述复合控制系统性能的特征参数。气动力回路控制对象含有一个离虚轴较近的非最小相位零点;而通过合理设计气动力控制器,直接侧向力控制对象只包含一个离虚轴较远的非最小相位零点,复合控制系统的跟踪性能可望比纯气动力的更好。设计实例对此进行了分析,揭示了非最小相位零点在控制器设计中的重要作用。 相似文献
783.
研究一种基于修正罗德里戈参数的考虑执行机构特性的飞行器滑模控制律.建立结合双框架控制力矩陀螺的飞行器姿态动力学模型和基于修正罗德里戈参数的姿态运动学模型;分析模型不确定性以判断其对滑模控制方法的适用性,提出滑动面进而设计相应的滑模控制器,接着结合线性系统理论和李雅普诺夫稳定原理对控制器的参数确定进行了分析;使用蒙特卡罗法数值仿真验证此控制律的效果.结果证明上述控制器可有效完成姿控任务,且控制精确,鲁棒性良好. 相似文献
784.
统计了某型液体火箭发动机涡轮泵27次地面试车振动数据和某型涡扇发动机28次台架试车振动数据,发现一次试车时间序列的振动特征参数随时间的波动反映了随机误差的变化,符合正态分布;不同台份发动机试车振动参数幅值的波动是发动机健康状态和试验误差共同作用的结果,不遵循正态分布规律,F分布是其分布的重要形式。在此基础上,研究了基于"概率相等法"和"3σ方法"原理的两种发动机振动限制值的确定方法。通过两种方法计算结果的相互验证,以及计算结果和工程实践的对比,说明确定振动限制值方法的正确性和实用性。 相似文献
785.
Da-Qi Xu Guo-Qiang Ni Li-Li Jiang Yuan-Ting Shen Ting Li Shu-Le Ge Xian-Biao Shu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(11):1800-1817
Reflectance spectra in the visible and near-infrared wavelengths provide a rapid and inexpensive means for determining the mineralogy of samples and obtaining information on chemical composition. Hydrocarbon microseepage theory establishes a cause-and-effect relation between oil and gas reservoirs and some special surface anomalies, which mainly include surface hydrocarbon microseepage and related alterations. Therefore, we can explore for oil, gas by determining reflectance spectra of surface anomalies. This idea has been applied to the R&D project of exploring for natural gas in Qinghai province of China using NASA EO-1 satellite with the Hyperion sensor (June 2005 to June 2006). In this project, in order to improve the accuracy of exploration targets of natural gas mapped in the field studied, an integrated practical system of exploration of oil and gas was built by the analysis of not only hyperspectral remote sensing data but also data provided from field work. In this paper, our efforts were focused on the analysis of the 799 reflectance spectra provided from the field work. In order to properly define the typical form of hydrocarbon microseepage with spectroscopy and fulfill the data analysis, it was necessary to build a spectral model. In this spectral model the most important features of hydrocarbon microseepage in the surface of our study area, i.e., diagnostic spectral macroscopic features and diagnostic spectral absorption features, were proposed and extracted, respectively. The distribution of coexisting anomalies, which results from both alteration minerals and hydrocarbons, is estimated by the diagnostic macroscopic features mainly using Spectral Angle Mapper (SAM) classifier. On the other hand, the diagnostic absorption features of two main absorption bands presented abundant local information, based on deep analysis of which, we are able to map the anomalies of alteration minerals and hydrocarbons, respectively. Additionally, a general framework of analysis and key classification algorithms applied to the Hyperion data have been introduced briefly. In our work, three exploration targets of natural gas were identified from the study area which covers 2100 km2. In the three exploration targets, three wildcats have been drilled by China National Petroleum Corporation (CNPC) since July 2006, and all the three wells have been proven some industrial reserves. 相似文献
786.
O.S. Oyekola Akin Ojo 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(9):1500-1509
The variability of the F2-layer even during magnetically quiet times are fairly complex owing to the effects of plasma transport. The vertical E × B drift velocities (estimated from simplified electron density continuity equation) were used to investigate the seasonal effects of the vertical ion drifts on the bottomside daytime ionospheric parameters over an equatorial latitude in West Africa, Ibadan, Nigeria (Geographic: 7.4°N, 3.9°E, dip angle: 6°S) using 1 year of ionsonde data during International Geophysical Year (IGY) of 1958, that correspond to a period of high solar activity for quiet conditions. The variation patterns between the changes of the vertical ion drifts and the ionospheric F2-layer parameters, especially; foF2 and hmF2 are seen remarkable. On the other hand, we observed strong anti-correlation between vertical drift velocities and h′F in all the seasons. We found no clear trend between NmF2 and hmF2 variations. The yearly average value of upward daytime drift at 300 km altitude was a little less than the generally reported magnitude of 20 ms−1 for equatorial F-region in published literature, and the largest upward velocity was roughly 32 ms−1. Our results indicate that vertical plasma drifts; ionospheric F2-layer peak height, and the critical frequency of F2-layer appear to be somewhat interconnected. 相似文献
787.
788.
针对耦合差分器件的散射参数测量,提出了一种使用对称反射标准件的混合模式TRL(Through-Reflect-Line)校准算法.根据过渡结构的多模散射矩阵元素之间的相位关系和散射矩阵的广义互易性,消除符号模糊性并得到过渡结构的混合模式转移矩阵.该算法要求的校准标准件类似于传统的单模式TRL算法,不需要非对称结构的反射标准件产生模式转换项.利用全波仿真方法得到了包含过渡结构的校准标准件和待测件的单模散射矩阵,并使用该算法对仿真数据进行处理,得到不包含过渡结构的待测件的混合模散射矩阵.将校准结果与不包含过渡结构的待测件的全波仿真结果进行比较,其一致性表明了该算法可有效地校准线性平衡器件. 相似文献
789.
Sudip Bhattacharyya 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
Measurement of at least three independent parameters, for example, mass, radius and spin frequency, of a neutron star is probably the only way to understand the nature of its supranuclear core matter. Such a measurement is extremely difficult because of various systematic uncertainties. The lack of knowledge of several system parameter values gives rise to such systematics. Low mass X-ray binaries, which contain neutron stars, provide a number of methods to constrain the stellar parameters. Joint application of these methods has a great potential to significantly reduce the systematic uncertainties, and hence to measure three independent neutron star parameters accurately. Here, we review the methods based on: (1) thermonuclear X-ray bursts; (2) accretion-powered millisecond-period pulsations; (3) kilohertz quasi-periodic oscillations; (4) broad relativistic iron lines; (5) quiescent emissions; and (6) binary orbital motions. 相似文献
790.