一种大变形多空间域连续体结构拓扑优化方法

针对大变形非线性结构拓扑优化问题,提出了基于混合细胞自动机(HCA, Hybrid Cellular Automata)多空间域连续体结构拓扑优化方法;采用密度法,建立了单元相对密度表示的材料弹-塑性模型;以单元相对密度和应变能作为细胞自动机(CA,Cellular Automata)的状态信息,利用CA局部控制规则,修改相对密度,迭代实现各设计空间域应变能均匀分布;设计了多空间域拓扑优化HCA算法,采取多个对象同时耦合优化迭代,各自收敛策略,解决了多空间域优化迭代算法收敛稳定性问题;最后,以汽车保险杆结构横梁和支撑等两个设计空间为例,施加大变形动态载荷作用,对提出的多空间结构优化算法进行了验证,优化后结构有效地降低了碰撞作用力峰值达54％,提高了结构安全性.     

Can identification of a fourth domain of life be made from sequence data alone, and could it be done on Mars?

A central question in astrobiology is whether life exists elsewhere in the universe. If so, is it related to Earth life? Technologies exist that enable identification of DNA- or RNA-based microbial life directly from environmental samples here on Earth. Such technologies could, in principle, be applied to the search for life elsewhere; indeed, efforts are underway to initiate such a search. However, surveying for nucleic acid-based life on other planets, if attempted, must be carried out with caution, owing to the risk of contamination by Earth-based life. Here we argue that the null hypothesis must be that any DNA discovered and sequenced from samples taken elsewhere in the universe are Earth-based contaminants. Experience from studies of low-biomass ancient DNA demonstrates that some results, by their very nature, will not enable complete rejection of the null hypothesis. In terms of eliminating contamination as an explanation of the data, there may be value in identification of sequences that lie outside the known diversity of the three domains of life. We therefore have examined whether a fourth domain could be readily identified from environmental DNA sequence data alone. We concluded that, even on Earth, this would be far from trivial, and we illustrate this point by way of examples drawn from the literature. Overall, our conclusions do not bode well for planned PCR-based surveys for life on Mars, and we argue that other independent biosignatures will be essential in corroborating any claims for the presence of life based on nucleic acid sequences.     

实时显示生成器

实时显示生成器(RTDB)是一种生成逻辑驱动显示的交互式图形工具样机。这些显示反映了当前系统状态,实时完成故障检测算法,采纳老练飞控人员的操作知识。该RTDB采用面向目标的方法,将基本操作逻辑和显示符号结合起来。要生成显示时,用户利用这种方法可规定屏幕布局和驱动逻辑。RTDB正在UNLX下用C语言开发,利用了MASSCOMP图形环境,作了适当的功能划分,以便于移植到其它图形环境。RTDB是为用户化实时数据驱动的航天飞机系统显示而开发的。使用该工具初始功能度的显示在STS—26发现者号轨道运行阶段投入了实用。目前正在NASA/JSC任务操作部开发的实时数据系统工程准备利用RTDB产生几种显示。本文介绍了这种工具的特点、目前的发展状况及其应用。     

跟踪与数据中继卫星系统的性能

一、引言 自60年代初,NASA就组建和操作一个为近地轨道卫星服务的跟踪和数据获取网。TDRSS是一个新测控网,为目前和直到2000年的预期卫星任务服务。该网利用了已经验证的空间和地面系统有关技术构成一个全新的测控站,只是其前端设备置于地球同步轨道上。尽量采用了自动化技术,使系统设置到数据采集以及整个跟踪期间的通信几乎都不需要人操作。     

陆军机动防空的发展趋势

地面部队的低空防空可分为保护固定发射场和机动设施两种.后者或者安装在机动车辆上限随机动部队进行,或者被牵引着用于保护构筑工事的部队.     

New results for the space radiation environment of MIR space station obtained by Liulin dosimeter-radiometer. Comparison with LET spectrometer NAUSICAA

Since 1988 high sensitivity semiconductor dosimeter-radiometer “Liulin” worked on board of MIR space station. Device measured the absorbed dose rate and the flux of penetrating particles. The analysis of the data hows the following new results:

In October 1989 and after March 24, 1991, two additional stable maximums in flux channel were observed in the southern-eastern part of South Atlantic Anomaly (SAA). These two maximums existed at least several months and seem to be due to trapped high energy electron and proton fluxes. In April 1991 additional maximums were localized in the following geographical coordinates regions: LATITUDE = (−35 °)–(−50 °) LONGITUDE = 332 ° − 16 ° and lat.(−46 °)–(−52 °) long. 360 ° − 60 °. Additional maximums diffusion occurs inside radiation belt. Appearance of these maximums seems to be closely connected with preceding powerful solar proton events and associated geomagnetic dynamics of new belt disturbances. After the series of solar proton events in June 1991 we observed significant enhancement of this new radiation belt formation. To achieve sufficient accuracy of dose rate predictions in low Earth orbits the structure and dynamics of new belt should be carefully analyzed to be included in a new environment model.

From the inter comparison of the data from “Liulin” and French developed tissue equivalent LET spectrometer NAUSICAA in the time period August–November 1992 we come to the following conclusions: Mainly there is good agreement between both data sets for absorbed dose in the region of SAA; Different situation of the instruments on the station can explain the cases when differences up to 2 times are observed; At high latitudes usually the tissue equivalent absorbed dose observations are 2 times larger than “Liulin” doses.     

含摩擦和加热的跨声速流动数值模拟研究

喷管中跨声速流动的反应流体动力学是实验和理论研究的一个重要领域.本文主要由两部分构成,在第一部分中对文献[2]中的Murman格式[1]的一般形式进行了简化,得到了守恒形式的欧拉方程,并对其求解方法进行了讨论,同时针对Chattot等的工作展开了分析,并给出了带激波的流动计算结果;而文章的第二部分则研究了包含摩擦、加热以及耗散的跨声速流动,并重点关注了一步Arrhenius化学反应模型下的爆震现象.本文还探究了摩擦力和带燃烧的跨声速流动之间的相互作用,同时详细给出了新的欧拉方程数值求解算法并同已有文献算例进行了对比验证.     

固体火箭发动机的实际和预示压力—时间历程之间的差别

固体火箭发动机(SRM_S)中实际的稳态压力——时间历程经常不遵循用经典方程和方法所预示的曲线形状。每个发动机偏离预示压力的最大幅度和时间均不相同。对具有圆柱和星孔形状的分段推进剂药柱的航天飞机固体火箭发动机,本文提出了关于这种偏差的数据。本文对端面燃烧药柱的有关类似情形的数据也进行了讨论。     

阿里安—4的固体助推器

本文介绍了阿里安—4固体助推器的结构和设计;详细地讨论了将阿里安—3的经验和试验结果改动最小地用于阿里安—4的结构设计问题;还介绍了研制和鉴定试验的详细结果。     

机载阵列雷达抑制运动杂波的学习算法

一种称为自适应空时处理器(STP)的线性滤波器是一种相对比较新的方法，它使机载阵列天线雷达目标检测概率达到最大。理论上，全自适应STP可以实时获得最优解(一种维恩滤波器)。但是，实际上全自适应STP也存在一些问题。首先，线性滤波器的加权数可能非常大。其次，单一加权矢量的计算复杂度大约为O(MN)^3。再次，STP为线性滤波器但却工作在非线性不稳定的环境中。这些问题导致采用空时处理器传统技术的实时、最佳处理是现行计算技术内所不及的。为使运动杂波对目标检测的影响最小，本文探讨了人工神经网络和几种学习算法的可应用性。人工神经网络是一种自适应、并行、分布式处理系统，可以实时完成复杂计算。学习算法的机理是为了存储新的信息或变更信息，人工神经网络中的长期存储器要不断更新而又不被破坏。由于学习算法既能在系统的使用期内保留信息又能变更信息，所以对雷达系统的计算要求降到了最低，同时还能适应环境的变化。