利用普通钻床或铣床加工高精度坐标孔

本文提供了一种用普通钻床加工高精度坐标孔的方法。提出了联合使用量块和一套导向镗孔装置的解决方案。     

Evolution of X-ray binaries: Achievements and advances

Three recent developments in the field of formation and evolution of neutron stars and black holes in binaries are addressed:

• The finding that there is a class of neutron stars, formed in interacting binaries, that do not receive kick velocities in their birth events. This finding is particularly important for our understanding of the formation – and formation rates – of double neutron stars. It is argued that these low-kick neutron stars, which tend to have low masses, are formed by a different physical mechanism than the neutron stars that receive large kick velocities at birth.

• The occurrence of velocity kicks in the formation events of stellar black holes.

• The nature of the companions of millisecond X-ray pulsars.

含孔有限大各向异性板的应力集中

 利用经典层板理论，将复合材料层板的弹性问题化归为均匀各向异性板求解，采用各向异性体平面弹性理论中的复势方法，以Ｆａｂｅｒ级数和最小二乘边界配置技术为工具，提出了含孔有限大层板应力集中问题的级数解，详细探讨铺层形式、层板大小、椭圆度等诸参数的影响。     

基于CCD的叶片气膜孔快速检测技术研究

研制了一套基于CCD的叶片气膜孔快速检测系统,采用机器视觉的方法,配合四轴测量机构,实现在叶片围绕轴线旋转的同时采集气膜孔的图像,然后利用Halcon图像处理算法库实现图像处理,并计算出气膜孔的尺寸参数。通过对某厂的叶片进行了测量实验,实现了对气膜孔轴线方向和直径的测量,弥补了气膜孔无法定性检测的技术空白,具有推广应用价值。     

冷却孔非均匀排布波纹板隔热屏冷却特性仿真

为了更加合理地分配冷却气体流量，提高纵向波纹板隔热屏结构的气膜冷却效率，提出了非均匀孔排布局波纹板隔热 屏结构，即保持开孔率不变，构建了上游波纹结构气膜孔排布密集、下游波纹结构气膜孔排布稀疏的非均匀结构。在发动机真实 工况下，采用数值仿真的方法研究了非均匀孔排方式对沿程冷却气体流量分配特性和气膜冷却特性的影响规律，揭示了振幅比变 化对波纹板隔热屏冷却效果的影响规律。结果表明：前密后疏型非均匀孔排布局可以改变冷却气体在隔热屏不同位置处的出流 量，从而显著提高隔热屏的气膜冷却效率。在气膜孔孔参数以及开孔率不变时，增大隔热屏上游孔排密度既可以提高隔热屏上游 的冷却效果，又不会明显降低隔热屏下游的冷却效果，使隔热屏整体面平均气膜冷却效率有所提高，相比于均匀孔排结构，前密后 疏孔排布局最高可使隔热屏面平均气膜冷却效率提高12.66%；在相同工况下，当振幅比从0.035增大至0.075时，隔热屏的面平均 气膜冷却效率显著提高，最高可使其面平均气膜冷却效率提高16.32%。     

发散冷却与冲击/发散冷却的冷却效率对比

为了得到最佳的冷却结构,在相同冷却气量下对发散孔单层壁与冲击/发散孔双层壁冷却结构的冷却效率进行了试验研究.试验保证相同的发散孔排布规律、热侧与冷侧进气温度、冷却气量、热气量以及热冷侧之间的空气压降,使用红外热像仪对发散孔壁的热侧壁面温度进行测量以得到冷却效率,并对两种结构的冷却效率进行对比分析.试验结果表明:在相同冷却开孔面积、相同冷热气条件下,冲击/发散孔双层壁的冷却效率要比发散孔单层壁大约高30%,这归因于冲击/发散冷却方式存在更高的换热强化能力.      

Delayed outburst of H 1743–322 in 2003 and relation with its other outbursts

The Galactic transient black hole candidate H 1743–322 exhibited a long duration outburst in 2003 after more than two and a half decades of inactivity. The 2003 event was extensively studied in multi-wavelength bands by many groups. The striking feature is that the total energy released is extremely high as compared to that in tens of outbursts which followed. In this paper, we look at this event and study both the spectral and temporal properties of the source using two component advective flow (TCAF) paradigm. We extract accretion flow parameters for each observation from spectral properties of the decay phase and determine the mass of the black hole. We computed the energy released during all the known outbursts since 2003 and showed that on an average, the energy release in an outburst is proportional to the duration of the quiescent state just prior to it, with the exception of the 2004 outburst. A constant rate of supply of matter from the companion cannot explain the energy release in 2004 outburst. However, if the energy release of 2003 is incomplete and the leftover is released in 2004, then the companion’s rate of matter supply can be constant since 1977 till date. We believe that erratic behaviour of viscosity at the accumulation radius $X_p$ of matter as well as location the $X_p$ itself, rather than the random variation of mass transfer rate from the companion, could be responsible for non-uniformity in outburst pattern. We discuss several factors on which the waiting time and duration of the next outburst could depend.     

精密盲孔珩磨工具设计技巧

介绍了影响盲孔珩磨精度的问题所在,根据平衡力矩原理,设计带有补偿油石磨损差值的珩磨工具,实现了在油石上下超程不相等的条件下,达到了对孔各部位的等量切削。     

Effect of dilution holes on the performance of a triple swirler combustor

A triple swirler combustor is considered to be a promising solution for future high temperature rise combustors. The present paper aims to study dilution holes including primary dilution holes and secondary dilution holes on the performance of a triple swirler combustor. Experimental investigations are conducted at different inlet airflow velocities(40–70 m/s) and combustor overall fuel–air ratio with fixed inlet airflow temperature(473 K) and atmospheric pressure. The experimental results show that the ignition is very difficult with specific performance of high ignition fuel–air ratio when the primary dilution holes are located 0.6H(where H is the liner dome height)downstream the dome, while the other four cases have almost the same ignition performance. The position of primary dilution holes has an effect on lean blowout stability and has a large influence on combustion efficiency. The combustion efficiency is the highest when the primary dilution holes are placed 0.9H downstream the dome among the five different locations.For the secondary dilution holes, the pattern factor of Design A is better than that of Design B.