关于CCSDS体制数据安全保护实施位置的探讨

主要阐述CCSDS（空间数据系统咨询委员会）标准的信息安全问题，重点是航天器安全，从分析空间数据面临的安全威胁出发，讨论了CCSDS不同安全实施位置的特点；并在此基础上，通过对CCSDS业务及数据结构的影响对比，总结出不同安全实施方法的优缺点，该结合对于采用CCSDS标准的空间数据系统如何解决信息安全问题，具有一定的参考价值。     

Series of radiation-hardened, high efficiency converters for high voltage bus

A review of common switching techniques for dc/dc power conversion is presented. The evolution of the forward converter is discussed, leading naturally to the introduction of the double forward converter. Technical details for a series of radiation-hardened converters are then provided. This series was designed for space power management and distribution (PMAD) applications. The successful development of the PMAD converter demonstrated the viability of high voltage bus.     

杠杆式力标准机自动控制系统

介绍单片机用于杠杆式力标准机控制、实现检定过程自动化的设计方法，重点介绍硬件结构和软件编制。     

关于一维非定常气─固二相流特征理论的讨论

本文研究了一维非定常气－团二相流的特征，对于目前常用的、包含一定近似的运动方程组，它有两个虚部很小的复根，研究表明这种很小的虚部出现与方程中引入的近似有关。从十多个算例的结果看，这样的虚部不影响人们在工程计算中用该方程组求解初值问题。针对具有上述特征的气－团二相流方程组，本文发展了一种类特征线方法，它保留了双曲型方程特征线方法的若干优点，但它允许方程的特征根中有微小的虚部。含灰气体激波管流动的计算表明，类特征线法具有精度高、数值耗散和弥散小等优点     

一种基于事件序列的故障树最小割集算法

在系统分析故障树最小割集各种求解算法的基础上，提出了一种故障树事件序列的数据结构，并针对该数据结构，设计了一种高效的故障树最小割集求解算法，并对其替换子算法、复制子算法和消减子算法进行了形式化描述。算法可有效降低最小割集生成中的“组合爆炸”问题，实验结果表明算法具有较好的计算性能。     

空间卫星目标动态电磁散射特性仿真与分析

给出了空间轨道飞行目标动态宽带散射特性建模方法,重点对某卫星动态宽带电磁散射特性进行了仿真,并通过轨道飞行过程中卫星一维距离像的积累获取了散射中心历程图,提出了由飞行过程中形成的散射中心历程图来判断卫星的结构特点的思路.     

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     

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.