凸轮逆序测量方法

目前各杂志所发表的关于凸轮测量的文章，所讨论的均是凸轮的顺序测量方法，有关凸轮的逆序测量(反求工程)方法，尚未见于文字。本文将对凸轮的逆序测量方法进行探讨。     

分布式计算机技术在飞机非标测控设备中的应用和实现

在研究、分析和总结分布式计算机技术与系统实现的基础上，以苏-27战斗机火控雷达天线部件性能测控系统研制过程为例，详细论述了分布式计算机测控系统的实现模式，介绍了一种先进合理的非标测控设备设计解决方案和快捷、低成本的系统实用集成方案。     

Physical characterization of the deep-space debris WT1190F: A testbed for advanced SSA techniques

We report on extensive ${\mathit{BVR}}_c{I}_c$ photometry and low-resolution ($\lambda /\mathrm{\Delta }\lambda ～250$) spectroscopy of the deep-space debris WT1190F, which impacted Earth offshore from Sri Lanka, on 2015 November 13. In spite of its likely artificial origin (as a relic of some past lunar mission), the case offered important points of discussion for its suggestive connection with the envisaged scenario for a (potentially far more dangerous) natural impactor, like an asteroid or a comet.Our observations indicate for WT1190F an absolute magnitude $R_c={32.45}_{\pm 0.31}$, with a flat dependence of reflectance on the phase angle, such as ${\mathit{dR}}_c/d?～{0.007}_{\pm 2}$?mag?deg^?1. The detected short-timescale variability suggests that the body was likely spinning with a period twice the nominal figure of $P_{\mathrm{flash}}={1.4547}_{\pm 0.0005}\mathrm{s}$, as from the observed lightcurve. In the ${\mathit{BVR}}_c{I}_c$ color domain, WT1190F closely resembled the Planck deep-space probe. This match, together with a depressed reflectance around 4000 and 8500 Å may be suggestive of a “grey” (aluminized) surface texture.The spinning pattern remained in place also along the object fiery entry in the atmosphere, a feature that may have partly shielded the body along its fireball phase perhaps leading a large fraction of its mass to survive intact, now lying underwater along a tight ($～1\times 80$?km) strip of sea, at a depth of 1500?m or less.Under the assumption of Lambertian scatter, an inferred size of ${216}_{\pm 30}/\sqrt{\alpha /0.1}$?cm is obtained for WT1190F. By accounting for non-gravitational dynamical perturbations, the Area-to-Mass ratio of the body was in the range $(0.006?\mathit{AMR}?0.011)$?m²?kg^?1.Both these figures resulted compatible with the two prevailing candidates to WT1190F’s identity, namely the Athena II Trans-Lunar Injection Stage of the Lunar Prospector mission, and the ascent stage of the Apollo 10 lunar module, callsign “Snoopy”. Both candidates have been analyzed in some detail here through accurate 3D CAD design mockup modelling and BRDF reflectance rendering to derive the inherent photometric properties to be compared with the observations.     

RAD-7测氡仪检定结果不确定度的评定

依据量值传递关系，列举了量值传递中的数学模型；依据数学模型，介绍了测氡仪检定结果不确定度的评定方法；结合JJG 825—2013《测氡仪检定规程》RAD-7的检定，评定出了RAD-7测氡仪检定结果体积活度响应的相对合成标准不确定度；结果表明，检定结果的不确定度主要受氡从液体镭源转移过程和被检仪器计数能力的影响。     

火星探测VLBI测定轨技术

我国将于2020年首次发射由环绕器和着陆巡视器组成的火星探测器,火星探测器的跟踪及精密测定轨是完成工程任务和科学探测的基础。火星探测器的跟踪和测定轨,目前主要采用基于地面无线电测量的测距、测速和甚长基线干涉VLBI测角3种手段。主要针对VLBI技术予以介绍,主要内容为:△DOR型VLBI技术在国内外的应用情况、火星探测器VLBI测定轨技术分析、基于同波束VLBI的火星车定位技术、火星探测器VLBI观测等。这些内容对我国的火星探测器测定轨有重要的应用价值。     

Microstructural characterization and mechanical behavior analysis of 7075-T6 aluminum subjected to simulated lightning strikes

Aircrafts damages caused by lightning strikes have been known since the early days of aviation. However, the physical effects on the aircraft structure are still being investigated. This work seeks to evaluate the lightning strike effects in the aluminum alloy 7075-T6. Samples were submitted to lightning strike simulation in laboratory and the damages evaluated through characterization techniques. Ultrasound and profilometry tests have shown material loss to 0.272 mm depth in the damaged region. In addition, it was detected the material accumulation occurrence in the damage vicinity of the region. Below the damage, it was found a region where metallurgical changes were identified. The tensile and microhardness tests results have shown reduction in the percentage elongation and hardness increasing in the material affected by lightning. These results are corroborated by the X-Ray Diffraction (XRD) and Rietveld Method (red line) that indicated an increasing in dislocation density and micro-deformation in the material matrix. Optical microscopy results have shown the presence of microcracks on the normal and cross-section surface of the samples damaged. The Energy Dispersive X-Ray Spectroscopy (EDXS) and Electron Backscattered Diffraction Test (EBSD) found coarse intermetallic phases and precipitates compounds with dimensions greater than 1 μm in length. They were responsible for nucleation of the microcracks that propagate along the material grain boundaries.     

基于检测结果的涡轮叶片精铸型腔反变形优化设计

针对空心涡轮叶片精铸过程中的试错法和数值仿真法难以敏捷反应铸件的真实变形情况,提出一种基于检测结果的精铸零件反变形综合补偿方法.通过对精铸叶片试模样件进行三坐标检测及统计分析,得到叶身截面收缩、扭转和弯曲变形情况,并建立其综合补偿反变形模具型腔优化算法,实现精铸型腔的反变形优化设计.以精铸叶片试模样件叶尖处截面为例,其叶身段型面误差、前缘最大误差、后缘最大误差相对于未补偿前分别减少了50%,68%和31%.实例验证表明:其研究成果能有效提高空心涡轮叶片的精铸成型精度,达到精确控形的目的.      

短距起飞/垂直降落发动机建模技术研究

参考常规双轴涡扇发动机数学模型,建立了适用于短距起飞/垂直降落(STOVL)飞机的变循环发动机部件级数学模型;通过特性外推,建立了轴驱动升力风扇数学模型;采用神经网络映射涵道总压损失的方法,建立了滚转喷管和外涵模型.根据STOVL发动机结构和部件变化特点,建立了稳态和动态共同工作方程.参照国外文献仿真数据进行设计点计算,并按照Bevilaqua提出方法开展了由常规涡轮风扇模式到悬停涡轮轴模式的过渡态仿真.仿真结果表明:建立的数学模型在悬停状态设计点和高空巡航点与国外文献数据相比误差均小于1.5%,推力达到悬停状态要求,符合STOVL发动机的设计特点,验证了该建模方法的有效性.      

光学坐标测量机的搭建与实现CSCD

为了高速高精高效地完成中小型复杂型面零件的测量,基于激光位移传感器和三坐标测量机等搭建了非接触式的光学坐标测量机,从而将测量机和光学测头的优点结合起来以应对空间自由曲面的测量任务。通过测头标定技术获得测量光束所在直线的单位方向向量,进而将激光测头的一维距离值转化为测量光斑的三维坐标值,然后通过坐标系转换将此坐标值转化到统一的测量机坐标系下,进而完成被测曲面三维点云的创建。最后,对一个直径已知的球在10个不同方位进行测量,通过点云数据拟合球面方程得到其直径作为测量结果,所得各次测量结果的误差均小于0.05mm,充分说明所搭建的测量系统的有效性。     

Search for high-proper motion objects with infrared excess

The possibility of interstellar migration has been theorized during the past thirty years in the form of “Dysonships” that, using non-relativistic propulsion systems, are able to colonize the Galaxy in a relatively short time compared to the age of the Galaxy and consequently penetrate inside our solar system too. Observational evidence of this can be potentially obtained using the present state of the art of telescopes and related sensors, by following aimed searches and an expanded SETI protocol. Some transient and unrepeated radio signals recorded during standard SETI observations might be due to the transit of high-proper motion artificial sources of extraterrestrial origin, which are expected to show a very weak optical emission, a strong infrared excess and occasional high-energy bursts in the X and Gamma-ray wavelength ranges. Such artificial sources might show an interest to Earth by sending probes to visit it: such a possibility can be investigated scientifically as well.