高速滚动轴承弹性流体动力润滑分析

直接采用弹性流体动力润滑（ＥＨＬ）分析方法计算了高速滚动轴承中滚子与内、外套圈接触区的油膜厚度、油膜动压力和润滑油牵引力;分析了载荷、转速及滚子数等参数对轴承打滑损伤的影响。理论分析结果与所作实验结果在较宽的工况范围内吻合较好。     

数字电路板故障诊断方法

介绍了数字电路故障诊断向量测试法中功能测试和在线测试的具体方法。结合现代武器系统数字电路板的检测和诊断需要,分别阐述了数字组合和时序电路板、数模混合电路板及微处理器电路板的故障诊断策略及步骤。举例说明了故障诊断方法在数字电路板自动测试系统中的应用。     

粉末激光烧结--一种广泛应用于工业生产的快速成形技术

~~粉末激光烧结——一种广泛应用于工业生产的快速成形技术$北京隆源自动成型系统有限公司@王科峰 $北京隆源自动成型系统有限公司@魏荣章 $北京隆源自动成型系统有限公司@侯细林 $北京隆源自动成型系统有限公司@柳国峰 $北京隆源自动成型系统有限公司@李建华~~     

The PROCESS experiment: an astrochemistry laboratory for solid and gaseous organic samples in low-earth orbit

The PROCESS (PRebiotic Organic ChEmistry on the Space Station) experiment was part of the EXPOSE-E payload outside the European Columbus module of the International Space Station from February 2008 to August 2009. During this interval, organic samples were exposed to space conditions to simulate their evolution in various astrophysical environments. The samples used represent organic species related to the evolution of organic matter on the small bodies of the Solar System (carbonaceous asteroids and comets), the photolysis of methane in the atmosphere of Titan, and the search for organic matter at the surface of Mars. This paper describes the hardware developed for this experiment as well as the results for the glycine solid-phase samples and the gas-phase samples that were used with regard to the atmosphere of Titan. Lessons learned from this experiment are also presented for future low-Earth orbit astrochemistry investigations.     

提高雷达测距精度的实用方法探讨

通过开展针对不同类型目标的雷达测距试验,得出雷达测距误差的一组数据。对其进行分析比较,总结出对于不同类型目标的雷达测距偏差产生的规律,给出了偏差的大致数量范围。     

Is the presence of oxygen on an exoplanet a reliable biosignature?

We revisit the validity of the presence of O(2) or O(3) in the atmosphere of a rocky planet as being a biosignature. Up to now, the false positive that has been identified applies to a planet during a hot greenhouse runaway, which is restricted to planets outside the habitable zone (HZ) of the star that are closer to the star. In this paper, we explore a new possibility based on abiotic photogeneration of O(2) at the surface of a planet that could occur inside the HZ. The search for such a process is an active field of laboratory investigation that has resulted from an ongoing interest in finding efficient systems with the capacity to harvest solar energy on Earth. Although such a process is energetically viable, we find it to be a very unlikely explanation for the observation of O(2) or O(3) in the atmosphere of a telluric exoplanet in the HZ. It requires an efficient photocatalyst to be present and abundant under natural planetary conditions, which appears unlikely according to our discussion of known mineral photochemical processes. In contrast, a biological system that synthesizes its constituents from abundant raw materials and energy has the inherent adaptation advantage to become widespread and dominant (Darwinist argument). Thus, O(2) appears to continue to be a good biosignature.     

Some ecological mechanisms to generate habitability in planetary subsurface areas by chemolithotrophic communities: the Río Tinto subsurface ecosystem as a model system

Chemolithotrophic communities that colonize subsurface habitats have great relevance for the astrobiological exploration of our Solar System. We hypothesize that the chemical and thermal stabilization of an environment through microbial activity could make a given planetary region habitable. The MARTE project ground-truth drilling campaigns that sampled cryptic subsurface microbial communities in the basement of the Río Tinto headwaters have shown that acidic surficial habitats are the result of the microbial oxidation of pyritic ores. The oxidation process is exothermic and releases heat under both aerobic and anaerobic conditions. These microbial communities can maintain the subsurface habitat temperature through storage heat if the subsurface temperature does not exceed their maximum growth temperature. In the acidic solutions of the Río Tinto, ferric iron acts as an effective buffer for controlling water pH. Under anaerobic conditions, ferric iron is the oxidant used by microbes to decompose pyrite through the production of sulfate, ferrous iron, and protons. The integration between the physical and chemical processes mediated by microorganisms with those driven by the local geology and hydrology have led us to hypothesize that thermal and chemical regulation mechanisms exist in this environment and that these homeostatic mechanisms could play an essential role in creating habitable areas for other types of microorganisms. Therefore, searching for the physicochemical expression of extinct and extant homeostatic mechanisms through physical and chemical anomalies in the Mars crust (i.e., local thermal gradient or high concentration of unusual products such as ferric sulfates precipitated out from acidic solutions produced by hypothetical microbial communities) could be a first step in the search for biological traces of a putative extant or extinct Mars biosphere.     

机翼低雷诺数流动的数值模拟

通过SIMPLE方法求解非定常不可压N-S方程,研究了小展弦比机翼在低雷诺数下的流场特征,并分析其对气动特性的影响。研究对象为展弦比为1.0的平板矩形翼,进行了不同攻角的数值模拟,模拟雷诺数为1×105。分析表明:在小攻角时,主涡不断的从机翼上表面脱落;在大攻角时,受翼尖涡的影响,分离涡保持在机翼的背风面不脱落,形成驻涡。通过对流场分析,低雷诺数前缘层流分离和翼尖涡对小展弦比机翼的空气动力学特性起了决定性作用;使低雷诺数小展弦比矩形翼出现非定常、非对称和驻涡等现象。     

中空长航时无人机两段翼型设计研究

中空长航时无人机存在高效巡航、短距起降以及抗变形等多性能要求,本文在原始飞机单段翼型的基础上,开展多约束条件下两段翼型设计方法研究和翼型设计。采用控制点加分段可控二次曲线方法构建两段翼型外形,并对生成外形的控制参数、缝道参数和转轴位置进行优化设计。分析结果表明:相比于常规直接切割法,本文采用的方法控制点和控制参数更多,对原始翼型适应性更好,生成的翼型压力分布更加合理;与原始翼型相比,新设计的两段翼型在续航因子、起飞升力和起飞升阻比方面得到大幅提升;同时襟翼大角度偏转还能起到阻力板作用,达到对巡航和起降多设计点综合设计要求。