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41.
郭祎  高力  王康 《导航与控制》2016,(6):95-100
针对现阶段石英加速度计零件的毛刺问题,分析了现有处理方法的缺陷.从被动去除和主动控制两条途径入手,以轭铁零件为例,在加工中引用了少无毛刺加工技术,并引进了新的去毛刺方法.强度检测结果表明,这两种方法的运用显著改善了毛刺控制的效果,值得推广和运用.  相似文献   
42.
本文研究了泵浦激光频率波动对核磁共振陀螺仪零偏稳定性的影响.通过分析核磁共振陀螺仪理论模型和自旋光泵浦极化129Xe的过程,阐述泵浦激光频率波动对陀螺仪零偏稳定性的影响机理.结果表明,泵浦光频率波动会导致核磁共振陀螺仪零偏稳定性下降约3个数量级.泵浦光频率波动是制约核磁共振陀螺仪性能提升的重要因素.  相似文献   
43.
提出了一种基于查表的开环记忆多项式模型(MPM,Memory Polynomial Model)预失真器.从MPM预失真器系数估计和执行信号预失真处理两方面加以考虑.首先,利用预失真器和高功率放大器(HPA,High Power Amplifier)传输特性的互补性,由采集到的HPA输入、输出基带数据进行单次最小二乘估计得到MPM预失真器的系数,避免了以往递归结构的收敛性和计算量大等问题.然后,利用MPM预失真器的特点,建立了基于输入信号强度索引的一维向量表,通过查表实现MPM预失真器的幂次累加项,极大地减少了实现预失真器所需的计算量及硬件开销.仿真显示,采用提出的预失真器可以有效补偿HPA对信号的记忆非线性失真,有效带宽内获得了近20 dB的功率改善,也显著改善了系统误码性能.  相似文献   
44.
We have studied the effect of both solar magnetic polarity and the solar wind velocity on the Bz-component of the interplanetary magnetic field, IMFBz, for the minimum activity of the solar cycles 21, 22, 23 and 24. We made a statistical study of IMFBz in the first section which is considered as an extension of Lyatsky et al. (2003). They made a statistical study of IMFBz for two periods of minimum solar activity 22 and 23 related to 1985–1987 and 1995–1997 when the solar magnetic field had opposite polarity. Our results seem to be consistent with the results obtained by Lyatsky et al. (2003). We found that there is a dependence of IMFBz on the IMFBx and the solar magnetic polarity for the minimum periods of the selected four solar cycles. In addition, we found that there is a dependence of IMFBz on the solar wind velocity.  相似文献   
45.
介绍了一种新研制开发的永磁吸附式双履带结构爬壁机器人,主要应用于火力发电站的大型排管锅炉中的水冷壁排管壁面的清扫和检测,并能够在检测到壁面厚度小于预置的极限值处发出报警信号、打标记,具有较高的推广应用价值。文中阐述了该机器人的结构、磁路的优化设计、自动测厚、打标系统和控制系统的研制。目前,该机器人已经经过多次现场试验。各项指标均已达到设计要求。  相似文献   
46.
航空航天智能材料与智能结构研究进展   总被引:2,自引:0,他引:2  
智能材料作为新兴多功能材料,能够实现结构功能化、功能多样化。智能结构是在结构中集成智能材料作为传感器和驱动器,使结构除了具有承载、传力、连接等功能外,还具有自感知、自诊断、自驱动、自修复等能力,以更好地适应外界环境的变化,可显著提升航空航天架构的性能。目前智能材料与智能结构已成为航空航天架构减重增效研究的重点。根据国内外智能材料和结构的研究进展,综述了压电材料、铁磁材料、形状记忆材料、智能复合材料等智能材料的发展;讨论了智能结构的研究及应用前景,包括自诊断智能结构、自修复智能结构和减振降噪智能结构;最后,指出了智能材料与结构当前面临的一些挑战性问题,展望了其在航空航天领域的应用前景。  相似文献   
47.
Abstract

Three experiments were conducted to examine whether people can adopt and maintain imagined perspectives in the absence of target information. The task used entailed providing information about an imagined perspective in advance of target information to examine whether this would facilitate perspective-taking performance and reduce or eliminate alignment effects that are commonly reported in the literature. The three experiments employed different types of spatial environments: an environment learned from navigating a computer screen (Experiment 1), and an immersive environment that was either remote (Experiment 2) or immediate (Experiment 3) at the time of retrieval. Across the three experiments, results showed that information about an imagined perspective can be utilized ahead of target information. Furthermore, they suggested that alignment effects can be reduced as a result of processing information about perspective ahead of target information, but only when reasoning about specific nonimmediate spatial relations (Experiments 1 and 2). Results are discussed in connection with previous findings on spatial updating and the organizational structure of spatial memory.  相似文献   
48.
Nowadays operational models for solar activity forecasting are still based on the statistical relationship between solar activity and solar magnetic field evolution. In order to set up this relationship, many parameters have been proposed to be the measures. Conventional measures are based on the sunspot group classification which provides limited information from sunspots. For this reason, new measures based on solar magnetic field observations are proposed and a solar flare forecasting model supported with an artificial neural network is introduced. This model is equivalent to a person with a long period of solar flare forecasting experience.  相似文献   
49.
就磁转速表活动系统的动态特性以及在附加交变力矩的作用下,指针摆动随转速变化的规律,从理论上进行了分析,并结合实际探讨了指针摆动的故障原因。  相似文献   
50.
Two orbits were selected in January–February 2006 when the separation between the Cluster spacecraft was large and mirror type magnetic field fluctuations were observed by all spacecraft in different regions of the terrestrial magnetosheath. Minimum variance analysis was applied to find the mirror type fluctuations, and the amplitude of the fluctuations was determined individually. Mirror mode structures are moving along the streamlines frozen in the plasma. A model was developed for the calculation of plasma flowtime from the bow shock to the observation point. The growth rate of the field strength perturbations was estimated by comparing the amplitudes of fluctuations observed simultaneously at distant locations (∼10,000 km) based on the assumption that δB ∼ exp(γt). The obtained growth rate values were about an order of magnitude smaller than those provided by linear models and they decreased in the inner regions of the magnetosheath, indicating some saturation in the growth of the waves when proceeding towards the magnetopause. The results of these two case studies suggest that mirror type fluctuations originate from the compression region downstream of the quasi-perpendicular bow shock, and the growth of the fluctuations cannot be described by linear approximations.  相似文献   
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