任意波发生器静态特性的评价

介绍了任意波发生器的主要静态特性指标、校准方法及实现过程。通过一组实验．获得了实际校准结果，并对校准中需要注意的问题进行了讨论。所述方法涉及的静态特性内容比较全面。具有足够的测量准确度、分辨力和稳定性。可用于任意波发生器的静态指标评价和计量。     

G-凸空间上的广义拟均衡问题

本文主要讨论局部G-凸空间上的均衡问题,得到一些结果。     

双主动交会远程导引方案建模与仿真

针对航天器双主动交会问题,以两航天器能量消耗之和最小为最优交会指标,建立了一种寻求远程导引可行飞行方案的算法模型,以满足远程导引对测控、日照和任务时间等要求。仿真结果表明,该算法可行。     

几种串行总线互连技术分析

随着计算机技术的发展,传统的并行总线已经不能满足日益增长的需求.简单介绍了新型的串行总线的一些特点、优势,并对现在几种流行的串行总线互连技术进行了比较分析,进行一些讨论.     

吸尘器弯管连接头模具的设计

分析了吸尘器弯管连接头的结构特点,着重阐述了应用于本模具中的一种新颖的专用来解决大角度,长距离抽芯的连杆机构的工作原理。对模具设计过程中遇到的困难,如:小嵌件如何固定,很小的侧型芯如何固定于侧滑块上,及三个液压缸按顺序抽芯,圆弧型芯如何插入圆柱型芯2中等都作了详细的叙述与探讨。另外本论文还涉及到了主要成型零部件的加工问题。     

rom 15 sel

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     

司马迁死因之谜新探

司马迁作为中国历史上伟大的史学家，其死因一直是千古之谜。是他杀还是自杀，从历史上的有关论述及当事人的思想性格等方面入手进行分析探究。     

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.