Kilohertz quasi-periodic oscillations in SAX J1808.4–3658

I present a short overview of the behavior and properties of the two simultaneous kilohertz quasi-periodic oscillations (kHz QPOs) seen in the accreting millisecond X-ray pulsar SAX J1808.4–3658. I will focus on the behavior of the upper frequency QPO as a function of time and count rate as seen during the 2002 outburst of this source. I will also discuss briefly the correlated behavior of this QPO with QPOs at lower frequencies (several tens of hertz).     

Broad-band spectral properties of accreting X-ray binary pulsars

Broad-band spectra of accreting X-ray binary pulsars can be fitted by a phenomenological model composed of a power law with a high energy rollover above 10 keV, plus a blackbody component with a temperature of few hundred eV. While, at least qualitatively, the hard tail can be explained in terms of (inverse) Compton scattering, the origin of the soft component cannot find a unique explanation. Recently, a qualitative picture able to explain the overall broad-band spectrum of luminous X-ray pulsars was carried out by taking into account the effect of bulk Comptonization in the accretion column. After a review of these recent theoretical developments, I will present a case study of how different modeling of the continuum affect broad features, in particular the cyclotron resonance features in Vela X-1.     

Appearance of neutron stars in the state of subsonic propeller

The state of subsonic propeller is intermediate between the states of supersonic propeller and accretor in the evolutionary tracks of magnetized compact stars. The rotational rate of a star at this stage decelerates due to the interaction between its magnetosphere and the surrounding hot, quasi-static plasma envelope. The magnetospheric radius is smaller than the corotation radius and the boundary of the magnetosphere is stable with respect to interchange instabilities. The rate of the mass flux from the inner radius of the envelope to the stellar surface is limited by the rate of plasma diffusion into the magnetic field of the star. As a result, the subsonic propeller would appear as a low-luminosity accretion-powered pulsar with a soft X-ray spectrum.     

转动旋翼模型动柔度的试验研究

介绍测定转动旋翼模型动柔度的试验方案、试验程序，综述以作者自行设计的旋翼模型进行试验所得到的结果及其与理论计算结果的比较。结果表明，试验方案与方法是可行的，理论计算公式是正确的。     

新型高推比涡轮风扇发动机盘时耦合振动分析

本文将群论算法和动态子结构技术结合起来，并采用计算效率极高的Ｂｅｎｆｉｅｌｄ－Ｈｒｕｄａ的模态代入变换法，分析了某型发动机压气机的叶片／轮盘耦合系统的振动特性，计算了该叶片／轮盘耦合系统的前５阶振动频率和振型．根据叶片／轮盘耦合系统的共振条件进行共振分析，确定该发动机压气机有可能发生叶片／轮盘耦合共振．     

同向旋转盘间换热特性的实验研究

本文将实际发动机高、低压涡轮盘简化成几何形状相对简单的中心轴向进气、径向出气、两盘以不同速度同向旋转的旋转盘系统。用实验方法研究了冷气流量、转速以及两盘间隙对旋转盘间换热的影响规律,并对结果进行了相应的分析。     

旋转环形截面弯管内流场结构及换热特性

环形截面弯管围绕其中心轴旋转时，同时受到科氏力和离心力作用，弯管内的对流换热更为复杂，本文对旋转环形截面弯管内的流动特性和温度分布进行了数值分析。结果表明：旋转环形截面弯管内的换热特性主要由Dn数，F数（科氏力和离心力之比),Pr数，和δ值（内外径之比）决定；文中给出并分析了在不同δ下流场结构与摩擦系数比随F数的变化特性和随Dn数的变化规律，并给出了在不同δ和Pr数情况下，温度场和管道Nu数随F数和Dn数的变化规律。     

高精密角度分度测量控制系统的研究

研制并开发了用于角度标定的高精密角度分度装置及其测量控制系统,装置采用永磁直流力矩电机驱动精密轴系主轴的运转来带动分度盘的转动,以圆光栅测量系统检测主轴的转动角度,为了实现角度的零误差分度定位控制,转动角度的分度控制采用了闭环自动控制系统。研究分析了圆光栅测量信号处理中信号细分形成的系统非线性误差对装置分度精度的影响,建立了误差修正模型,通过误差补偿,系统在±5°的角度测量范围内分度控制精度达到±0.2″。     

InSb磁敏电阻角位移传感器的研究

简单分析了InSb磁敏电阻的工作原理，讨论了利用偏置磁场作用于半桥磁敏电阻构成转动速度及位移传感器的测试原理；针对半导体材料对温度十分敏感的特点，提出了利用浮动零点跟踪技术测试齿轮转速的方法，并对其优缺点进行了讨论。     

大型转动机械碰摩故障分析的声发射检测系统

汽轮发电机、空气压缩机等采用油膜支撑的大型转动机械,由于安装或运行中的原因,在转子旋转过程中,可能和器壁发生轻微的摩擦和碰击,简称碰摩.声发射技术在碰摩发生特别是故障早期诊断上有优越性.本系统的特点是没有沿用传统的计数、幅度、能量和持续时间等声发射特性参数,而是在声发射包络信号的频率分析中进行特征提取.声发射发生的过程分析和现场试验都表明这种方法对碰摩检测很敏感,在碰摩发生的起始阶段,包络谱中与转速同步的周期性分量显著增加.根据这种新的设计思想自行研制了BUAA碰摩声发射检测仪并对此作了介绍.