The case for massive,evolving winds in black hole X-ray binaries

In the last decade, high-resolution X-ray spectroscopy has revolutionized our understanding of the role of accretion disk winds in black hole X-ray binaries. Here I present a brief review of the state of wind studies in black hole X-ray binaries, focusing on recent arguments that disk winds are not only extremely massive, but also highly variable. I show how new and archival observations at high timing and spectral resolution continue to highlight the intricate links between the inner accretion flow, relativistic jets, and accretion disk winds. Finally, I discuss methods to infer the driving mechanisms of observed disk winds and their implications for connections between mass accretion and ejection processes.     

波音737NG飞机前货舱后隔板下部支撑横梁腐蚀受损分析及改进

某航空公司波音737NG机队飞机前货舱后隔板下部支撑横梁腐蚀严重,受损率较高,如不及时更换将发生变形甚至断裂,影响周围其他重要结构部件甚至影响飞行安全,但更换该部件成本较高。统计表明,其受腐蚀损坏程度与机龄、密封、首次检查期限和重复检查间隔等因素相关。严格执行检查和提高维护标准可以降低维修成本,若进一步改进支撑梁底部密封,可延长其使用寿命。     

鲁棒的结构网格自动化重叠方法

网格技术是目前数值模拟中的关键技术之一。重叠网格是一种放宽拓扑要求、减小网格生成难度的网格技术。本文以结构重叠网格为基础,分别针对挖洞、寻点以及洞面优化方法进行了研究和改进,同时完成物面网格重叠,形成了一套鲁棒的、自动化的网格重叠系统。在挖洞方面,结合“最小洞映射”方法,提出“复合式挖洞”方法,节省内存开销;在寻点方面,通过构建格心虚网格,保证搜索空间的连续性,同时结合“有效搜索”思想,排除部分对寻点无贡献的网格点,进而减少ADT叉树节点;在洞面优化上,改变填补判别法则并引入两类受保护洞内点,确保两层插值边界建立,提高鲁棒性;在物面网格重叠上,利用物面投影法完成坐标修正,实现物面附近网格流动变量的准确传递。为验证本文方法,分别对定常翼身组合体DLR-F6绕流和非定常机翼挂载分离过程进行了数值模拟,计算结果与实验结果吻合良好,表明该结构重叠网格系统对多物体间定常、非定常扰流具有较好的数值模拟能力和较高的模拟精度,具有较高的工程应用价值。     

复合材料单排多钉连接三维累积损伤强度分析

机械连接是复合材料结构的主要连接形式,针对复合材料层合板单排多钉双剪联接接头,建立了静拉伸三维累积损伤模型,考虑了多种最终失效判定准则;考虑了单排钉不同的几何尺寸。结合有限元技术即应力分析、失效判定准则、损伤后材料性能退化及机械连接最终失效准则,对复合材料机械连接接头部位在静载作用下的累积损伤失效过程及各钉孔孔径的变化过程进行模拟分析。用该模型预测的结果与试验结果进行了比较分析,数值分析结果与试验结果比较一致。     

基于故障统计模型的导弹武器系统贮存检测周期确定方法

综合运用可靠性工程理论、现代数理统计理论等,以实际故障统计数据为基础,提出了确定导弹贮存检测周期的方法,并用Matlab进行了计算验证.     

一种Ka频段波导微带鳍线转换结构

为使波导微带转换的尺寸和性能更优,采用HFSS高频仿真软件里的样条曲线做波导微带转换的鳍线渐变曲线,使波导微带转换的过渡长度与采用其他渐变曲线在相同指标情况下相比更短一些。转换模型中的介质基片向标准矩形波导宽边两侧延伸四分之一波长并在其上各打一行孔径和间距合适的金属填充通孔,这样既便于固定基片,又能提高鳍线电路的隔离度。使用HFSS软件对该模型进行仿真优化分析后的结果为：在28．5～39GHz频带内得到大于25dB的回波损耗和小于0．1dB的插入损耗,基本达到预期目的。     

钛合金螺旋铣孔孔径偏差研究

螺旋铣孔是航空航天领域新出现的制孔技术,其切削过程中会产生径向切削力,从而引起刀具变形并造成孔径偏差。针对该问题开展了钛合金螺旋铣孔孔径偏差试验,分析了包括进给方向在内的不同加工参数对孔径偏差的影响规律;基于螺旋铣孔运动学原理对不同进给方向下的材料去除过程和径向切削力方向进行了研究,分析了不同进给方向下的孔径偏差变化规律及形成原因,并设计切削力试验进行了验证;通过分析不同加工参数下的未变形切屑形状及径向切削力变化情况,研究了各加工参数对孔径变化趋势的影响规律。研究结果表明,当进给方向为顺时针时,刀具受背离孔心的径向切削力的作用向孔径外侧发生挠曲变形,导致所加工孔径大于理论孔径;当进给方向为逆时针时则相反。进给速度和导程的增加将加剧孔径偏差,切削速度的增加则会减弱孔径偏差。     

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.     

一起典型的FJ44-1A发动机金属末故障分析

航空发动机滑油系统发现金属末意味着这发动机部件之间出现了过度磨损,这类故障严重影响飞行安全,必须查明故障原因并纠正。本文根据多次发动机热端部件检查的实践经验,对一起由于安装不当造成发动机轴承磨损的故障进行了分析,并总结了FJ44-1A发动机热端部件装配的若干经验。     

Constraining the mass of the black hole GX 339-4 using spectro-temporal analysis of multiple outbursts

We carried out spectro-temporal analysis of the archived data from multiple outbursts spanning over the last two decades from the black hole X-ray binary GX 339-4. In this paper, the mass of the compact object in the X-ray binary system GX 339-4 is constrained based on three indirect methods. The first method uses broadband spectral modelling with a two component flow structure of the accretion around the black hole. The broadband data are obtained from RXTE (Rossi X-ray Timing Explorer) in the range 3.0 to 150.0?keV and from Swift and NuSTAR (Nuclear Spectroscopic Telescope Array) simultaneously in the range 0.5 to 79.0?keV. In the second method, we model the time evolution of Quasi-periodic Oscillation (QPO) frequencies, considering it to be the result of an oscillating shock that radially propagates towards or away from the compact object. The third method is based on scaling a mass dependent parameter from an empirical model of the photon index ($\mathrm{\Gamma }$) – QPO ($\nu$) correlation. We compare the results at 90 percent confidence from the three methods and summarize the mass estimate of the central object to be in the range $8.28–11.89M_{\odot }$.