Estimating the spin axis orientation of the Echostar-2 box-wing geosynchronous satellite

For the first time, the spin axis orientation of an inactive box-wing geosynchronous satellite has been estimated from ground-based optical photometric observations of Echostar-2’s specular reflections. Recent photometric light curves obtained of Echostar-2 over four years suggest that unusually bright and brief specular reflections were occurring twice within an observed spin period. These bright and brief specular reflections suggested two satellite surfaces with surface normals separated by approximately 180°. The geometry between the satellite, the Sun, and the observing location at the time of each of the brightest observed reflections, was used to estimate Echostar-2’s equatorial spin axis orientation coordinates. When considering prograde and retrograde rotation, Echostar-2’s spin axis orientation was estimated to have been located within 30° of either equatorial coordinate pole. Echostar-2’s spin axis was observed to have moved approximately 180° in right ascension, within a time span of six months, suggesting a roughly one year spin axis precession period about the satellite’s angular momentum vector.     

低频声波对水雾消散作用的实验研究

作者考查了低频声波(<50Hz)对于水雾消散的作用。通过建立声波消雾实验装置,测定了在水雾消散过程中,雾室内的声场分布、温度、消雾时间、雾滴谱的变化过程。实验结果表明声波作用对于水雾的消散具有明显的作用。并且,消雾的效果随着作用声波的频率和声压级(SPL)呈规律性的变化趋势。较低频率和较高声强的声波作用更有利于水雾的消散,在消雾的过程中温度起伏不大。而声致凝聚是声波消雾的主要因素之一。     

中原城市群经济发展水平及空间布局研究

中原城市群位于我国东西部的经济缓冲带，尚处于发展的初始阶段。采用多元统计分析方法，通过对选取的13项经济指标进行定量研究，分别得到了中原城市群在河南省的经济发展水平排名与城市群经济发展相似程度分组，从而得到河南省经济发展水平的空间分布表。结果表明：（1）中原城市群在河南省的总体经济发展水平中居于核心地位，但单个城市优势尚不明显，且存在较大差异；（2）中原城市群经济发展相似程度的空间分布有很强的聚集特征；（3）群内城市分别与群外城市在经济发展上呈现有规律的阶梯分布，且城市群在河南省的总体梯度较高；（4）城市群经济发展水平空间布局与地理位置、资源状况、经济基础紧密相关。结合上述实际情况，河南省应当依托中原城市群，把工作重点放在以下三个方面：（1）进一步突出首位城市郑州对周围城市的带动作用，建设以郑州为中心的城市圈；（2）缩小群内城市的经济水平差异和不平衡性，加快经济发展一体化进程；（3）在推进产业一体化的同时，注重发挥各自特色，形成合理的产业布局。     

SHS法制备硼化物陶瓷粉体的表征分析

采用自蔓延高温还原合成方法制备TiB2,TiB2-Al2O3和ZrB2-Al2O3陶瓷粉末.利用XRD,XPS,SEM以及TEM等分析测试手段对合成粉末进行表征和分析.结果表明,TiB2,ZrB2和Al2O3分别以主晶相的形式存在于所合成的各自粉体之中.相比之下,TiB2单相陶瓷粉末颗粒分布较宽.由于自蔓延高温合成(SHS)温度很高,部分颗粒形成团聚,宏观上使颗粒的平均粒径变大(＞5μm);而TiB2-Al2O3和ZrB2-Al2O3复合陶瓷粉末,因合成过程中Al2O3的形成,使得颗粒粒度分布明显变窄,分布均匀,颗粒尺寸也相应减小.分析认为这主要与复合粉末合成过程中,不同颗粒间形成良好结合的界面有关.     

无损检测的内涵演变及其在质量控制中的作用

就无损检测的内涵如何从探伤演变到评价及无损检测在质量控制中的应有作用作了叙述,希望对相关人员开拓思路、提高工作质量有所裨益.     

二元冰蓄冷测试技术及其评价

对二元冰蓄冷系统的测试技术进行了系统的介绍并作出了相应的评价。着重介绍了二元冰的性质及系统中凝聚现象和含冰率的测试技术,为二元冰蓄冷系统的测试研究指明了方向。     

航空用铝合金超微结构实验表征

为了使铝合金更好的服役于航空领域,就有必要对其微观结构进行实验表征,从而可以在铝合金微观结构和宏观性能之间搭建桥梁,最终优化铝合金的综合性能。本文介绍了航空用2xxx,6xxx和7xxx系铝合金发展历程以及时效析出过程中的微观结构演变,如Al-Cu合金GP区、Al-Cu-Mg合金GPB区等重要物相的结构特征,以及AlCu-Mg合金S相析出行为等都已得到了透彻的研究;阐述了透射电镜、扫描透射电镜、三维原子探针等技术的结合在Al-Cu-Mg-Ag合金Ω相、Al-Mg-Si-Cu合金β″相的晶体结构及界面结构以及铝合金晶间腐蚀机理等研究上的应用;本小组实现了复杂选区电子衍射谱的快速模拟及标定,并基于会聚束电子衍射实现了对析出相体积分数的精确测量;最后指出,高分辨透射电镜原位加热研究及透射电镜原位力学测试等新技术手段的应用,对深层次研究铝合金相变规律、变形行为具有跨时代意义。     

基于锥形压入的材料力学性能测试方法研究

通过压入测试以获取工程服役结构、小型构件和焊接结构焊缝过渡区的材料单轴本构关系参数,且根据材料本构关系参数来估算材料的压入硬度对于工程设计和安全评估有重要意义.对于幂律材料,本文依据锥形压入试验原理和弹塑性接触有限元分析(EPFEA),揭示了不同锥角的锥形压头其压入能量比与屈服应力之间存在线性关系,提出了基于能量原理预测金属材料本构关系部分关键参数(弹性模量、屈服应力和硬化指数)的CR-EMI (Constitutive Relationship based on Energy Method of Indentation)方法.同时,基于此种线性关系提出了由Hollomon本构关系模型参数预测硬度的H-EMI(Hardness based on Energy Method of Indentation)方法.通过对多种金属材料进行压入试验和有限元分析,验证了CR-EMI方法和H-EMI方法的有效性与精确性.     

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.     

Ti—15—3合金时效性能研究

研究了不同炉号的Ｔｉ－１５－３（Ｔｉ－１５Ｖ－３Ｃｒ－３Ｓｎ－３Ａｌ）合金时效温度、时间以及Ａｌ当量与力学性能的关系。在５００～５４０℃范围内拉伸强度与时效温度呈线性关系,平均斜率为－３ＭＰａ／℃。得出了强度与Ａｌ当量的线性方程式,推算出最佳Ａｌ含量为３．１％～３．３％。采用统计方法研究了强度与塑性关系,并研究了冷加工对时效性能的影响。研究的达到１０８０ＭＰａ强度级别的５２０℃／１０ｈ／ＡＣ的时效制度具有满意的力学性能,并应用于制造飞机阻力伞梁。