基于鸽群优化算法的实时避障算法

为保证机器人能安全无碰撞地抵达目标位置，提出一种在改进版圆形扩张（CSE+）法中融合鸽群优化算法的实时避障算法。所提算法引入对障碍物密集程度的判断机制，在障碍分布密集时选择最安全的路径，在障碍物分布稀松的环境中，利用鸽群优化算法在安全范围内寻找下一目标最优位置。此外，还引入了搜索树，可实现死角的检测与避免。仿真结果显示:所提避障算法能提高路径规划的性能，在障碍物分布稀松时效果更加明显，且可实现死角检测并能通过狭长通道。      

电铸镍Wolter I型光学系统制造技术发展综述

摘要： 为满足未来脉冲星导航和空间天文观测任务对X射线望远镜的载荷需求，Wolter I光学系统的研制正逐渐成为新的研究热点，电铸镍方案是当前国内外X射线光学系统镜筒制造的主要技术方案.文章对电铸镍X射线光学系统制造工艺、国内外研制现状、未来应用需求进行了介绍和整理，梳理了电铸镍X射线光学系统研制遇到的关键技术和难点，提出了后续研究发展建议，以促进中国在 X射线脉冲星自主导航、空间探测领域的快速发展.     

The LM-2C/SMA Launch Vehicle under Preparation for Launch

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电子工作台在模拟电子技术中的应用

本文简要地介绍了电子工作台的特点和使用方法，结合我们设计具体模拟电子线路的实践，说明了电子工作台在模拟电子技术中的应用。     

航空工业发展中存在的问题与对策——以河南省为例

重视发展战略、重视国内市场、重视技术创新以及重视对外合作是航空工业发达国家发展航空工业的主要经验.我国航空工业目前存在着企业规模小、布局分散、"软实力"不足、产品多属民品、科研体制存在弊端等问题.加速我国航空工业的发展,需要制定长远的发展规划,以市场为导向,加大结构调整力度,进行一系列的体制机制创新以及重视现有航空产品的改进改型,广泛进行国际国内合作,等等.     

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with primary goat embryonic fibroblast showed no difference from traditional feederlayer-based culture method used in mouse and human. The putative primary EG colonies were multilayer clumps ofcompact cel     

现场动平衡技术在生产中的应用

利用美国恩泰克公司提供的DP1500数据采集仪及现场动平衡软件,以实例说明了现场动平衡技术在锅炉引风机、排粉风机、电动机、机泵等转动设备不平衡故障排除中的应用,介绍了不平衡故障的识别方法,揭示出该技术在生产中的实用性、先进性和经济性.     

计算机帧时间对半实物仿真的影响

半实物仿真试验中,要求计算机帧时间与计算积分步长相一致,但在实际试验中不容易精确地做到。本文分析了这种不一致给半实物仿真试验带来的影响,给出了解决的办法,文章中还给出了一实例来说明。     

Field formation around negatively biased solar arrays in the LEO-plasma

Heavy emission caused by impacting plasma ions results in a fast discharging effect of the initially large surface potentials on the dielectric solar cells. This eventually counteracts the energization process of the plasma ions to the cover glasses and leaves no significant electric fields. Thus, with an existing thermal plasma, electrons are again able to reach dielectric surfaces. Strong localized electric fields of the order of several 10 kV/cm form near the interconnector-cover glass interface.     

EUV emission from normal galaxies

Using data from the Wide Field Camera EUV all-sky survey, we have established upper limits to the EUV flux from a sample of 30 bright, nearby, non-active spiral galaxies. These galaxies were chosen to be those most likely to be detected in the EUV on the basis of (i) low interstellar absorption within our own galaxy, (ii) brightness in other wavebands, (iii) high star formation activity, and (iv) proximity. The derived EUV upper limits are restrictive, and establish for the first time that the EUV flux escaping from galaxies does not constitute a major component of their bolometric luminosity, and in particular that it cannot be the sink for the energy injected into the interstellar medium by supernova explosions, as had been suggested following the failure to detect this power in the X-ray band.