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211.
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213.
倪国芬 《航空精密制造技术》2014,(6)
介绍了在感应同步器作为精位置反馈元件的转台使用中,为实现实时仿真而设计的测控电路,并给出了原理分析与实践结果。 相似文献
214.
系留气球在近地面收放过程中存在俯仰角过大的问题,为了更全面地了解收放过程中不同因素对球体俯仰角的影响,采用LMS Virtua1. Lab建立了带滑轮索具系统的系留气球三维动力学模型进行仿真分析,结果表明,仿真结果与理论计算、测量数据都有较高的符合度。进而运用试验设计( DOE)方法,探索典型风速下球体俯仰角的响应区间。最后基于响应面模型的优化技术,对滑轮索具系统设计进行优化,有效改善了球体在收放过程中俯仰角过大的问题。仿真模型对系留气球系统设计及收放控制有一定的指导作用。 相似文献
215.
采用了理论设计和有限元仿真分析相结合的方法,设计了基于液体静压导轨的大行程快刀伺服系统(最大加工行程30mm,行程4mm时频响不低于50Hz).首先,设计得到了基于液体静压导轨的大行程快刀伺服系统的结构模型和相关参数;接着,利用ANSYS/FLUENT软件对液体静压导轨的变形、模态以及油膜压力分布进行仿真分析,并且将油膜刚度的理论计算值和仿真计算值进行比较,验证了导轨设计的可靠性;最后,选用能够满足要求的音圈电机、位置反馈装置以及功能强大的MPAC运动控制器等完成了控制系统的搭建. 相似文献
216.
针对独立运行的导弹制导半实物仿真试验系统接入联合试验系统的问题,应用了仿真代理的方法。在对原有系统控制关系进行最小化的改造前提下,通过控制接口的转换,实现了半实物仿真试验系统与其它异类异构系统之间的互联,拓展了半实物仿真试验系统的应用。 相似文献
217.
Mikhail Sachkov Boris Shustov Ana Ines Gómez de Castro 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
During last three decades, astronomers have enjoyed continuous access to the 100–300 nm ultraviolet (UV) spectral range where the resonance transitions of the most abundant atoms and ions (at temperatures between 3000 and 300 000 K) reside. This UV range is not accessible from ground-based facilities. The successful International Ultraviolet Explorer (IUE) observatory, the Russian ASTRON mission and successor instruments such as the Galaxy Evolution Explorer (GALEX) mission or the COS and STIS spectrographs on-board the Hubble Space Telescope (HST) prove the major impact of observations in the UV wavelength range in modern astronomy. Future access to space-based observatories is expected to be very limited. For the next decade, the post-HST era, the World Space Observatory – Ultraviolet (WSO–UV) will be the only 2-m class UV telescope with capabilities similar to the HST. WSO–UV will be equipped with instruments for imaging and spectroscopy and it will be a facility dedicated, full-time, to UV astronomy. In this article, we briefly outline the current status of the WSO–UV mission and the science management plan. 相似文献
218.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(2):739-744
We examine the state of seven southern radio sources at the time of their RadioAstron AGN Survey observations. Both ATCA flux density monitoring data and Fermi light-curves are considered in determining the relative activity of the source. A simple hypothesis, that sufficiently compact source structure exists for detections on RadioAstron baselines when the source is in a flaring state, is qualitatively tested. We find four instances of RadioAstron detections during flaring radio states and four instances of RadioAstron non-detections during fading or quiescent radio states, in support of the hypothesis. However, we also find three instances of RadioAstron detections during quiescent or fading radio states, and two non-detections during a flaring state, indicating that the situation is (not unexpectedly) more complex. Radio and gamma-ray monitoring such as that described here, together with the full RadioAstron AGN Survey results, will allow a more thorough investigation of the dependencies of detections on baselines of >10 Earth diameters. 相似文献
219.
220.
This paper deals with geometric error modeling and sensitivity analysis of an overconstrained parallel tracking mechanism. The main contribution is the consideration of overconstrained features that are usually ignored in previous research. The reciprocal property between a motion and a force is applied to tackle this problem in the framework of the screw theory. First of all, a nominal kinematic model of the parallel tracking mechanism is formulated. On this basis, the actual twist of the moving platform is computed through the superposition of the joint twist and geometric errors. The actuation and constrained wrenches of each limb are applied to exclude the joint displacement. After eliminating repeated errors brought by the multiplication of wrenches, a geometric error model of the parallel tracking mechanism is built. Furthermore,two sensitivity indices are defined to select essential geometric errors for future kinematic calibration. Finally, the geometric error model with minimum geometric errors is verified by simulation with SolidWorks software. Two typical poses of the parallel tracking mechanism are selected, and the differences between simulation and calculation results are very small. The results confirm the correctness and accuracy of the geometric error modeling method for over-constrained parallel mechanisms. 相似文献