基于立体视觉的孔探分析系统及其应用

孔探分析在现代航空发动机故障诊断中一直发挥着重要的作用，开发基于立体视觉的孔探分析系统，对提高故障诊断水平和预测准确度，节约发动机维护成本有着重要的现实意义，系统利用立体视觉技术以及图像处理技术，完成了对双目视觉左右图像的标定和匹配，实现了对实体表面的三维测量和立体重建，本文介绍了基于立体视觉的孔探分析系统的基本原理与主要功能，并结合应用实例验证了系统的有效性。     

用Radon变换迭代法重建含有遮挡物的三维折射率场

本文通过计算机模拟研究，结合气体折射率场的光验知识．考查了将Ｒａｄｏｎ变换迭代法用于光学干涉层析计量含有遮挡物的三维折射率场的重建精度。作为一个应用实例，测量和计算了某一截面的气体温度分布，并与热电偶测量的值进行了比较。     

New multifrequency measurements of the spectrum of the cosmic background radiation

New measurements of the Cosmic Background Radiation temperature at 12 cm, 6.3 cm, 3 cm, 0.9 cm and 0.3 cm have made in July 1982 from the White Mountain High Altitude Research Station. The results are presented and the existence of spectral distortions discussed.     

Families of halo orbits in the elliptic restricted three-body problem for a solar sail with reflectivity control devices

Solar sail halo orbits designed in the Sun-Earth circular restricted three-body problem (CR3BP) provide inefficient reference orbits for station-keeping since the disturbance due to the eccentricity of the Earth’s orbit has to be compensated for. This paper presents a strategy to compute families of halo orbits around the collinear artificial equilibrium points in the Sun-Earth elliptic restricted three-body problem (ER3BP) for a solar sail with reflectivity control devices (RCDs). In this non-autonomous model, periodic halo orbits only exist when their periods are equal to integer multiples of one year. Here multi-revolution halo orbits with periods equal to integer multiples of one year are constructed in the CR3BP and then used as seeds to numerically continue the halo orbits in the ER3BP. The linear stability of the orbits is analyzed which shows that the in-plane motion is unstable while the out-of-plane motion is neutrally stable and a bifurcation is identified. Finally, station-keeping is performed which shows that a reference orbit designed in the ER3BP is significantly more efficient than that designed in the CR3BP, while the addition of RCDs improve station-keeping performance and robustness to uncertainty in the sail lightness number.     

抗辐射保偏光纤的制备及其特性研究

通过对保偏光纤进行光漂白与低温相结合处理的方式，来提高光纤的抗辐射性能。保偏光纤再经过1.0 kGy的高剂量预辐照处理后，其损耗会明显增大。随后采用980nm的激光对光纤进行光漂白处理,其损耗并没有发生明显变化。但是，处理后的样品在小剂量辐照条件下其光纤传输呈现先减小后增大的趋势。对于通过液氮进行冷处理的预辐照样品，其光纤传输损耗得到明显的降低，同时光纤经过小剂量辐照后的损耗同样也具有先减小后增大的现象。最后，将两种处理方式相结合，一方面可以有效地降低预辐照光纤的传输损耗，另一方面也使得保偏光纤在小剂量辐照的条件下，使其传输损耗具有减小的趋势，大大提高了保偏光纤在小剂量辐照条件下的抗辐照特性。     

外翼上壁板根部连接形式对飞机承载能力的影响研究

在飞机结构设计中,外翼上壁板根部连接处结构形式对飞机的传力、变形、承载能力具有重要影响.通过对3种不同形式的上壁板根部连接方案进行压缩试验,研究各方案的承载能力、破坏方式.通过三维有限元方法,计算了连接部位的主要螺钉所分配的载荷,研究了长桁根部斜角对结构屈服载荷的影响,得到了最优的选型方案.     

纤维增韧陶瓷基复合材料的比例极限应力与残余热应力关系

从细观力学角度分析并建立了纤维增韧陶瓷基复合材料从制备温度冷却到室温过程中产生的残余热应力与复合材料的比例极限应力的关系模型。该模型表明,减少复合材料的残余热应力或提高复合材料的纤维与基体的模量比,均可提高复合材料的比例极限应力。通过单调拉伸实验测试了先驱体浸渍裂解法(PIP)制备的2D SiC/SiC复合材料的比例极限应力,并采用文中建立的比例极限应力与残余热应力关系模型,计算出复合材料SiC基体的残余热应力为-19.5 MPa。分析表明,该结果是合理的。此外,引用了公开文献报道的5种复合材料体系数据,用于验证文中所建立的比例极限应力与残余热应力关系模型的适应性和可靠性,计算结果与实验结果最大误差为18.6%,表明该模型具有较好的适应性和可靠性,可为纤维增韧陶瓷基复合材料的研究提供新思路。     

某型航空活塞发动机曲轴喷油螺钉的维修工艺研究

喷油螺钉是某型航空活塞式发动机曲轴组合中的重要零件，单纯采用超声波清洗难以清除该零件内部积炭。结合生产实践对工艺进行改良，使该零件修理后的抽检合格率由20%提升至70%，缩短了发动机的翻修时间，节约了维修成本。     

硅氮烷环体的催化聚合及热解制备Si3 N4 材料

采用甲基氢二氯硅烷的氨解产物硅氮烷环体(MHSZ)为原料,以四丁基氟化铵为催化剂,制备了高分子量的硅氮烷聚合物(PHSZ),结合红外、核磁、凝胶色谱仪和热重分析了反应时间对合成的PHSZ结构、组成、分子量和陶瓷产率的影响。考察了低温氨气,高温N2气氛处理工艺对热解产物结构和组成的影响。结果表明,随着反应时间的延长,PHSZ高聚物的分子量提高,热失重降低;采用该热解方式PHSZ可转化为含碳量仅为0.5wt%的Si3N4材料,热解样品在1 600℃时完全结晶,晶相主要是α-Si3N4。     

Global ionospheric scintillations revealed by GPS radio occultation data with FY3C satellite before midnight during the March 2015 storm

Global observations of S4 amplitude scintillation index by the GPS Occultation Sounder (GNOS) on FengYun-3 C (FY3C) satellite reveal global dynamic patterns of a strong pre-midnight scintillations in F-region of the ionosphere during the St. Patrick’s Day geomagnetic super storm of 17–19 March 2015. The observed strong scintillations mainly occurred in the low latitudes, caused by equatorial plasma bubbles. During the main storm phase (March 17), the scintillations were first triggered in the New Zealand sector near 160°E longitudes, extending beyond 40°S dip latitude. They were also enhanced in the Indian sector, but significantly suppressed in East Asia near 120°E longitude and in Africa around 30°E longitude. During the initial recovery phase (March 18–19), the global scintillations were seldom observed in GNOS data. During the later recovery phase (after March 19), the scintillations recovered to the pre-storm level in Indian, African, and American sectors, but not in East Asian and any of Pacific sectors. These results closely correlate with observations of the density depletion structures by the Communication/Navigation Outage Forecasting System (C/NOFS) satellite, and ground-based instruments. Such consistency indicates reliability of our scintillation sensing approach even in a case-by-case comparison study. The prompt penetration electric field and disturbance dynamo electric field are suggested as the main factors that control the enhancement and inhibition of the scintillations during the storm, respectively.