Theoretical and Experimental Analysis on Influence of Revolution Radius in Orbital Drilling

Revolution radius is one of the significant parameters in orbital drilling,which has great influence on many factors,such as the cutting area of front and side cutting edge,undeformed chip geometry,delamination and burr at hole exit side,hole surface roughness,cutting tool force and deflection,chip removal and heat transmission.First,the influence of revolution radius on the factors is discussed theoretically in detail.Analysis results show that big revolution radius can reduce axial cutting force,restrain exit delamination and burr,and improve chip removal and heat transmission.Then,single factor test and orthogonal test are utilized in the two processing methods as machining unidiameter holes with several cutting tools and machining different diameter holes with one tool.Finally,the influence of revolution radius on cutting force and hole machining precision is studied.These results provide a profound foundation for future optimization of cutting control parameters.     

非晶态薄带冷却铜辊用内反馈静压轴承数值模拟

由于内反馈式静压轴承具有高回转精度、大承载能力和高油膜刚度等特性,固将其引入到非晶态薄带冷却铜辊支承结构中。为了获取冷却铜辊用内反馈静压轴承的承载能力特性,利用流体力学软件建立不同偏心距下的内反馈式静压轴承油膜模型,研究不同进油压力下随偏心距变化时轴承油膜压力场分布情况并计算出其承载能力。结果表明：在同等进油压力下,油膜承载能力随偏心距的增大而增大;在同等偏心距下,油膜承载能力随进油压力的增大而增大。最终通过与工作现场实验数据比对分析,当进油压力分别为3.0 MPa和3.5 MPa时,数值模拟载荷值与实际载荷值的相对误差分别为5.3%和5.4%,证明了数值模拟结果的可靠性。     

Performance comparison of aero-ramp and transverse injector based on gas-pilot flame

A direct performance comparison between the four-hole aero-ramp injector and single transverse injector in a dual-mode scramjet combustor was conducted. The mixing characteristics of two injectors were calculated by solving the three-dimensional (3-D) compressible Reynolds-averaged Navier-Stokes equations (RANS), with the help of the shear-stress-transport (SST) k-ω turbulence model. The numerical results show that the far field mixing efficiency of the aero-ramp injector is higher than that of the single transverse injector. High enthalpy vitiated air was heated to a total temperature of 1200K by hydrogen-oxygen combustion, entering the isolator entrance at a Mach number of 2.0. Non-reacting experimental conditions involved sonic injection of nitrogen to safely simulate ethylene injected into the combustor at a jet-to-free stream momentum flux ratio of 2.6. Schlieren photographs were obtained to analyze the shock structure around the injectors. Reacting test conditions involved sonic injection of ethylene at the jet-to-free stream momentum flux ratios ranging from 0.5 to 2.7. High speed camera was used to capture the flame structures in the near-field combustion. The experimental results show that the aero-ramp injector produce sustained combustion over a wider range of fuel-air ratios than the single transverse injector. At the identical jet-to-free stream momentum flux ratio, the aero-ramp has a larger isolator margin than the single transverse injector, demonstrating a better ability for avoiding overflows. However, the air specific impulse and total temperature recovery of two injectors, which are calculated by the one-dimensional (1-D) performance analysis code, are almost identical.      

适用于月面高温环境的嫦娥三号地形地貌相机热设计

“嫦娥三号暠月面探测器上安装的地形地貌相机工作时直接暴露在月面高温环境下,受月表红外辐射影响很大,给热控设计带来很大难题。为解决设备工作时的高温问题,在外热流分析的基础上提出了以“最佳散热位置暠为核心的热控方案,设备处于“最佳散热位置暠时能够获得较好的初始温度和最快的降温速率;另外通过把散热面布置在月表红外辐射热流最小的位置并在除散热面以外的其他表面包覆多层隔热组件这两个措施,可以最大程度减小月表红外辐射的影响。地形地貌相机在轨开机工作前的各飞行阶段遥测数据均满足存储温度指标要求并且有较大余量;开机工作环拍一周的遥测数据满足工作温度指标要求并且与热分析结果符合较好,初始温度与遥测温度数据偏差为-1灡7曟,温升速率和降温速率偏差分别为14灡9%和16灡9%。这表明该热控方案正确可行,可为后续中国深空探测类似热控问题参考。     

超（近）临界压力航空煤油RP-3的拟过冷沸腾传热特性

为了研究吸热型碳氢燃料在新型飞行器中的再生冷却性能,采用电加热方式,在热流密度0.1-1.0MW/m2和质量流速500-1000kg/m2s条件下,小通道圆管内（D=1.6mm）研究了超（近）临界压力下（P=3MPa）航空煤油RP-3的拟沸腾流动传热特性。研究发现了超（近）临界压力航空煤油的拟过冷沸腾传热现象。拟过冷沸腾壁温变化特征和传热恶化特征与亚临界压力下的相应特征存在差异。超临界压力航空煤油传热区域划分为类液态强制对流传热区、拟过冷沸腾区和类气态强制对流传热区。拟过冷沸腾壁温和传热系数随流体温度增加而缓慢增加,起到传热强化的作用;拟临界温度区域,存在传热系数极小值点,燃料发生传热弱化;燃料温度大于拟临界温度,燃料处于超临界类气态,传热大幅强化。     

高海况下反舰导弹对舰船目标攻击策略

反舰导弹攻击海面舰船目标时,通常根据目标的散射特征数据进行目标类型判定并做出决策。但是在高海况下:如果导弹横浪飞行,海浪对导弹命中目标的影响会变小,基本能保证可靠命中目标;但如果导弹顶浪飞行,则海浪会引起目标雷达反射截面积(Radar Cross Section,RCS)的起伏甚至突变,影响导弹对目标的锁定和判断。文章建立了不同海况和舰船目标的融合模型,并针对融合模型仿真计算了导弹不同突击方向时的 RCS,最终根据高海况时舰船横浪或顶浪航行的原则,按照捕捉概率最大的方向确定导弹的攻击方向。     

三波长数字相位解调法解调误差及影响因素

介绍了光纤法布里-珀罗(F-P)传感器的传统解调方法,系统地推导了针对非本征法布里-珀罗干涉型(EFPI)传感器解调的三波长数字相位解调法的解调原理,仿真和实验分析了三波长数字相位解调法的解调误差。仿真分析结果表明,相位偏离正交关系是限制解调的最主要因素,要保证解调误差在15 nm以内,腔长变化应小于在正交腔长处2μm的范围。采用3个独立的激光光源进行实验,实验结果表明,在正交腔长附近1μm范围内变化,解调腔长误差小于12 nm,重复性误差小于10 nm,解调具有良好的稳定性。     

高超声速风洞WDPR支撑尖锥模型应用可行性分析

绳牵引并联机构(WDPR)能够有效调整飞行器模型的位姿,为扩展风洞试验能力提供了一种新型支撑手段,具有很大的应用潜力。本文将对其在高超声速风洞中应用所涉及的稳定性与气动干扰问题进行研究。以10°尖锥标椎模型为例,设计了8绳牵引的并联支撑系统,可以通过调整绳长控制模型的位置和姿态。模拟了气动载荷作用下支撑系统的稳定性,优化牵引绳直径。基于构建的三维模型,借助CFD软件进行气动计算,包括马赫数为7.8时,不同迎角下绳牵引并联支撑锥体模型的气动力系数,通过与无绳支撑结果以及文献试验数据进行比较,表明在小迎角情况下,绳系支撑引起的气动干扰相对误差较小,但会随迎角的增大而增加。此外,分别对弯刀支撑和绳牵引并联支撑进行了模态分析,对比了2种支撑的固有频率。结果显示绳系支撑固有频率较高,系统刚度较大。本文的理论研究成果可为绳牵引并联支撑技术在高超声速风洞中的应用提供一定的技术支持。     

Super-resolution reconstruction of astronomical images using time-scale adaptive normalized convolution

In this work, we describe a new multiframe Super-Resolution (SR) framework based on time-scale adaptive Normalized Convolution (NC), and apply it to astronomical images. The method mainly uses the conceptual basis of NC where each neighborhood of a signal is expressed in terms of the corresponding subspace expanded by the chosen polynomial basis function. Instead of the conventional NC, the introduced spatially adaptive filtering kernel is utilized as the applicability function of shape-adaptive NC, which fits the local image structure information including shape and orientation. This makes it possible to obtain image patches with the same modality, which are collected for polynomial expansion to maximize the signal-to-noise ratio and suppress aliasing artifacts across lines and edges. The robust signal certainty takes the confidence value at each point into account before a local polynomial expansion to minimize the influence of outliers. Finally, the temporal scale applicability is considered to omit accurate motion estimation since it is easy to result in annoying registration errors in real astronomical applications. Excellent SR reconstruction capability of the time-scale adaptive NC is demonstrated through fundamental experiments on both synthetic images and real astronomical images when compared with other SR reconstruction methods.