混合电路仿真的新方法

实际的数字系统均由数字电路和模拟电路组成，分析数字电路的方法与分析模拟电路的方法是完全不同的。本文将给出一种仿真混合电路的新方法及相应的模拟器。ＭＣ－ＳＩＭ的主要原理如下：首先把被模拟电路划分成许多模拟模块和数字模块，模拟（数字）模块只有模拟（数字）输出；任一模拟输入均视一系列发生在离散的时间点上的事件；模拟模块在达到之前与数字模块一样参加排队；不论是数字模块还是模拟模块都在统一的时间轮下进行计算     

离心机微机监控系统的模拟调试

结合介绍国家七·五项目“离心机微机监控设备”的模拟调试，论述了实验室或现场模拟调试的重要性；研究了模拟调试的内容和被物理、电子模拟装置替代的实际系统中的对象的分类；探讨了如何设计与制作一个或若干个既简单又“逼真”的模拟调试辅助装置，建立一个高效率的模拟调试环境。     

载人火星探测的行星保护

行星保护是影响载人火星探索任务的重要问题之一。载人探测的行星保护包括3个方面,即防止来源于地球的微生物污染目标星球的正向污染防护、防止外来生物对地球的潜在危害的逆向污染防护,以及确保航天员的健康和安全。国际宇航界已经开始针对载人火星探测的行星保护制定政策法规和开展技术研讨。本文介绍了行星保护的定义和法理依据,简要回顾了美国国家航空航天局在“阿波罗登月”中的行星保护措施,并对未来载人火星探测中的主要污染物、污染途径以及污染防护策略进行了初步探讨。     

一种支持 NF￣2 和多媒体的数据模型

支持ＮＦ２（Ｎｏｎ－ｆｉｒｓｔ－ｎｏｒｍａｌ－ｆｏｒｍ）和多媒体的数据库系统ＮＦＭＤＢ是在关系数据库ＲＤＢＭＳ的基础上研制的,它是一种扩充了的ＤＢＭＳ。系统采用了扩充的关系数据模型,它支持ＮＦ２和多媒体的数据存储和数据操作。本文重点介绍了ＮＦＭＤＢ系统支持ＮＦ２和多媒体的数据模型,以及基于数据字典的实现方案,系统具有处理复杂对象的能力。     

实时数据库的主动机制研究与实现

主动机制是实时数据库管理系统（ＤＢＭＳ）的一个重要功能。在主动机制的基础上,实时ＤＢＭＳ能够根据数据库中某些数据及环境的变化,主动地作出一定的反应,执行预先设计的动作,而不仅仅是被动地执行用户的命令。文中主要介绍一个实时ＤＢＭＳ的主动子系统,采用事件－条件－动作的规则来实现其主动功能;讨论了规则的表示和存储结构,规则子系统的系统结构及与ＤＢＭＳ的联系;并详细介绍了条件评价器、规则检索优化、规则冲突     

格栅翼减阻特性研究

为了探索减少格栅翼阻力的方法和途径 ,进行了超声速M∞ =2 .5 2 1下格栅翼的边框几何形状和尺寸以及格栅翼茎厚度、格栅几何形状对格栅翼阻力特性影响的风洞实验。结果显示 ,格栅翼的边框对格栅翼的阻力影响最大 ,选择合适的边框厚度和剖面形状可以有效地减少格栅翼的阻力     

Volatile Trapping in Martian Clathrates

Thermodynamic conditions suggest that clathrates might exist on Mars. Despite observations which show that the dominant condensed phases on the surface of Mars are solid carbon dioxide and water ice, clathrates have been repeatedly proposed to play an important role in the distribution and total inventory of the planet’s volatiles. Here we review the potential consequences of the presence of clathrates on Mars. We investigate how clathrates could be a potential source for the claimed existence of atmospheric methane. In this context, plausible clathrate formation processes, either in the close subsurface or at the base of the cryosphere, are reviewed. Mechanisms that would allow for methane release into the atmosphere from an existing clathrate layer are addressed as well. We also discuss the proposed relationship between clathrate formation/dissociation cycles and how potential seasonal variations influence the atmospheric abundances of argon, krypton and xenon. Moreover, we examine several Martian geomorphologic features that could have been generated by the dissociation of extended subsurface clathrate layers. Finally we investigate the future in situ measurements, as well as the theoretical and experimental improvements that will be needed to better understand the influence of clathrates on the evolution of Mars and its atmosphere.     

模态法辨识针刺C/ C 复合材料弹性模量

针对传统方法测量C/ C 复合材料弹性模量精度差问题,提出了一种利用模态试验辨识材料弹性 模量的新方法。数值仿真结果表明板件材料振动频率与弹性模量之间存在模糊对应关系,利用此关系采用二 分法及二阶响应面近似模型对材料弹性模量进行辨识,并分别利用各向同性薄壁板件及正交各向异性薄壁板 件对此方法进行验证,计算结果误差最大为16. 67%,最小仅为0. 5%,表明该方法准确有效。最后将其应用于 针刺C/ C 复合材料,获得了其弹性模量。仿真及试验结果均表明该方法无损、高效且准确度高。     

复合材料机尾罩减重设计

根据复合材料层压板及夹层结构设计原则提出了某飞机机尾罩复合材料设计方案,结合复合材料强度计算方法进行有限元分析及强度校核。分析结果表明:在满足静强度的前提下,与金属机尾罩相比,复合材料机尾罩重量减少28.4%。     

Potential Effects of Surface Temperature Variations and Disturbances and Thermal Convection on the Mars InSight HP<Superscript>3</Superscript> Heat-Flow Determination

The HP³ instrument on the InSight lander mission will measure subsurface temperatures and thermal conductivities from which heat flow in the upper few meters of the regolith at the landing site will be calculated. The parameter to be determined is steady-state conductive heat flow, but temperatures may have transient perturbations resulting from surface temperature changes and there could be a component of thermal convection associated with heat transport by vertical flow of atmospheric gases over the depth interval of measurement. The experiment is designed so that it should penetrate to a depth below which surface temperature perturbations are smaller than the required measurement precision by the time the measurements are made. However, if the measurements are delayed after landing, and/or the probe does not penetrate to the desired depth, corrections may be necessary for the transient perturbations. Thermal convection is calculated to be negligible, but these calculations are based on unknown physical properties of the Mars regolith. The effects of thermal convection should be apparent at shallow depths where transient thermal perturbations would be observed to deviate from conductive theory. These calculations were required during proposal review and their probability of predicting a successful measurement a prerequisite for mission approval. However, their uncertainties lies in unmeasured physical parameters of the Mars regolith.