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基于快速模糊干扰观测器的UASV再入Terminal滑模控制 总被引:2,自引:1,他引:2
针对无人空天飞行器再人大气层过程中气动参数变化剧烈、控制精度要求高的特点,设计了基于快速模糊干扰观测器的Terminal滑模控制方案。通过改进传统模糊干扰观测器的学习律,提出一种快速模糊干扰观测器,增强了其在线逼近干扰及系统不确定的能力。Terminal滑模的有限时间收敛特性提高了系统跟踪速度,同时采用快速模糊干扰观测器消除全部扰动的影响,从而保证了飞行品质。最后,仿真结果表明了快速模糊干扰观测器的优越性及闭环控制方案的有效性。 相似文献
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D. Martini K. Mursula T. Ulich V.S. Pandey K.-H. Kim D.-H. Lee 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
Here we compare the traditional analog measure of geomagnetic activity, Ak, with the more recent digital indices of IHV and Ah based on hourly mean data, and their derivatives at the auroral station Sodankylä. By this selection of indices we study the effects of (i) analog vs. digital technique, and (ii) full local-time vs. local night-time coverage on quantifying local geomagnetic activity. We find that all other indices are stronger than Ak during the low-activity cycles 15–16 suggesting an excess of very low scalings in Ak at this time. The full-day indices consistently depict stronger correlation with the interplanetary magnetic field strength, while the night-time indices have higher correlation with solar wind speed. The Ak index correlates better with the digital indices of full-day coverage than with any night-time index. However, Ak depicts somewhat higher activity levels than the digital full-day indices in the declining phase of the solar cycle, indicating that, due to their different sampling rates, the latter indices are less sensitive to high-frequency variations driven by the Alfvén waves in high-speed streams. On the other hand, the night-time indices have an even stronger response to solar wind speed than Ak. The results strongly indicate that at auroral latitudes, geomagnetic indices with different local time coverage reflect different current systems, which, by an appropriate choice of indices, allows studying the century-scale dynamics of these currents separately. 相似文献
206.
Bang-Zhao Zhou Guo-Ping Cai Yun-Meng Liu Pan Liu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(1):207-222
Capturing a non-cooperative space target is a tremendously challenging research topic. Effective acquisition of motion information of the space target is the premise to realize target capture. In this paper, motion prediction of a free-floating non-cooperative target in space is studied and a motion prediction algorithm is proposed. In order to predict the motion of the free-floating non-cooperative target, dynamic parameters of the target must be firstly identified (estimated), such as inertia, angular momentum and kinetic energy and so on; then the predicted motion of the target can be acquired by substituting these identified parameters into the Euler’s equations of the target. Accurate prediction needs precise identification. This paper presents an effective method to identify these dynamic parameters of a free-floating non-cooperative target. This method is based on two steps, (1) the rough estimation of the parameters is computed using the motion observation data to the target, and (2) the best estimation of the parameters is found by an optimization method. In the optimization problem, the objective function is based on the difference between the observed and the predicted motion, and the interior-point method (IPM) is chosen as the optimization algorithm, which starts at the rough estimate obtained in the first step and finds a global minimum to the objective function with the guidance of objective function’s gradient. So the speed of IPM searching for the global minimum is fast, and an accurate identification can be obtained in time. The numerical results show that the proposed motion prediction algorithm is able to predict the motion of the target. 相似文献
207.
基于聚类模糊系统的动态数据野值剔除方法 总被引:1,自引:0,他引:1
针对影响遥测参数处理和分析的野值问题,提出了基于聚类法实时设计模糊系统实现动态数据野值辨识和剔除的新方法。该方法能够自适应跟踪不同变化特性的遥测参数,基于聚类法实现模糊系统的动态建模并获得预测值与观测值的残差序列,再按照狄克松准则实现野值的快速剔除。对实测数据的仿真实验表明:该方法能够显著降低动态建模的复杂度,快速跟踪信号变化,方法可行且有效。 相似文献
208.
K.K. Singh J. Singh M. Altaf Ashutosh K. Singh S. Kumar A.K. Singh Shyampati Lalmani 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
The purpose of this paper is to describe some unusual whistlers (doublets and triplets) and VLF hiss emission recorded simultaneously on February 18, 1998 during nighttime at a low latitude Indian ground station Jammu (geomag. lat., 22° 26′ N; L = 1.17), and to make some discussions about their origin. The detailed structures of the observed VLF hiss emission clearly show that these emissions confined to a narrow continuous frequency band. Some times the frequency of hiss band oscillates and subsequently touches the upper edge of the first whistler component of the doublet. Detailed structures of the dynamic spectra of whistler and VLF hiss emission are briefly presented. From the dispersion analysis of the whistler doublets and triplets, it is found that the individual whistlers of the doublets and triplets simultaneously observed on the same day are one-hop whistlers having propagation path along higher and closely spaced L-values. Our result also shows that VLF hiss has been generated in the equatorial region of higher L-values. Generation and propagation mechanisms are briefly discussed. 相似文献
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城市污水处理厂污泥热解机理 总被引:1,自引:0,他引:1
本研究采用热重分析仪对南昌市青山湖污水污泥进行热重分析实验,分别获得了20 K/min和40 K/min加热速率下污泥的TG-DTG曲线,得出了污水处理厂污泥的热解特性。根据实验结果对干燥污泥热解过程进行了分析且利用积分法确定了热解机理,求出反应动力学参数-频率因子A、活化能E。 相似文献