空间光学精密展开机构展开方法的初步探讨

文章对空间光学精密展开机构(以下简称展开机构)进行分类,分析了几种典型可展开空间光学系统的展开方法和特点。讨论了展开机构设计需要考虑的主要因素,并给出设计建议。     

中板加热炉高效燃烧控制系统

介绍了控制系统在热值比较稳定的前提下,依靠控制加热炉排气中的残氧量以降低空燃比,达到降低排气热损失的目的,实现了加热炉节能降耗.     

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.     

Spectra and time variability of black-hole binaries in the low/hard state

We propose a jet model for the low/hard state of galactic black-hole X-ray sources which explains the energy spectra from radio to X-rays and a number of timing properties in the X-ray domain such as the time lag spectra, the hardening of the power density spectra and the narrowing of the autocorrelation function with increasing photon energy. The model assumes that (i) there is a magnetic field along the axis of the jet, (ii) the electron density in the jet drops inversely proportional to distance, (iii) the jet is “hotter” near its center than at its periphery, and (iv) the electrons in the jet follow a power-law distribution function. We have performed Monte Carlo simulations of Compton upscattering of soft photons from the accretion disk and have found power-law high-energy spectra with photon-number index in the range 1.5–2 and cutoff at a few hundred keV, power-law time lags versus Fourier frequency with index 0.8, and an increase of the rms amplitude of variability and a narrowing of the autocorrelation function with increasing photon energy as they have been observed in Cygnus X-1. The spectrum at long wavelengths (radio, infrared, optical) is modeled to come from synchrotron radiation of the energetic electrons in the jet. We find flat to inverted radio spectra that extend from the radio up to about the optical band. For magnetic field strengths of the order 10⁵–10⁶ G at the base of the jet, the calculated spectra agree well in slope and flux with the observations.     

Modeling the broadband persistent emission of magnetars

In this paper, we discuss our first attempts to model the broadband persistent emission of magnetars within a self-consistent, physical scenario. We present the predictions of a synthetic model that we calculated with a new Monte Carlo 3D radiative code. The basic idea is that soft thermal photons (e.g. emitted by the star surface) can experience resonant cyclotron upscattering by a population of relativistic electrons treated in the twisted magnetosphere. Our code is specifically tailored to work in the ultra-magnetized regime; polarization and QED effects are consistently accounted for, as well different configurations for the magnetosphere. We discuss the predicted spectral properties in the 0.1–1000 keV range, the polarization properties, and we present the model application to a sample of magnetars soft X-ray spectra.     

The beaming of external Compton emission

We consider a relativistically moving blob consisting of an isotropic electron distribution that Compton-scatters photons from an external isotropic radiation field. We compute the resulting beaming pattern, i.e. the distribution of the scattered photons, in the blob frame as well as in the observer’s frame by using the full Klein–Nishina cross section and the exact incident photon distribution. In the Thomson regime the comparison of our approach with Dermer (1995) results in concurrent characteristics but different absolute number of the scattered photons by a factor of f_corr = 3.09. Additionally, our calculation yields a slightly lower boost factor which varies the more from the corresponding value in Dermer (1995) the higher the spectral index p of the electron distribution gets.     

Z-pins增强陶瓷基复合材料层间Ⅰ型开裂性能预测

基于Z-pins增强陶瓷基复合材料层间Ⅰ型断裂韧性的试验结果、Z-pins增强机理,提出了Z-pins拔出的单线性软化模型.重点考虑了Z-pins直径范围内拔出位移的不一致性,在简单双悬臂梁（DCB）理论的基础上,获得了Z-pins增强陶瓷基复合材料层间Ⅰ型开裂性能的分析预测模型,预测结果与试验结果吻合较好.在此基础上,采用预测模型获得了不同Z-pins直径、裂纹长度下的裂尖能量释放率,并与理想弹簧元法进行了比较.结果表明:当裂尖靠近Z-pins时,随着Z-pins直径增大,两种方法所得的裂尖能释放率的差异逐渐增大,但总体来说差异的量级很小;随着裂纹长度的增加,裂尖逐渐远离Z-pins,两种方法所得的裂尖能释放率的存在较大的差异,不能忽略Z-pins直径范围内拔出位移不一的影响.      

加温超载处理对提高30CrMnSiA钢构件裂纹扩展寿命的作用

对带裂纹的３０ＣｒＭｎＳｉＡ钢紧头等拉伸试件进行同时加温超载处理，经卸载冷却后，在裂纹端区产生残余压应力塑性场。这一处理方法起到延缓裂纹扩展、抑制起裂的效果。     

含闭链机构机器人动力学探讨

本文用Appell方程就含闭链机构机器人动力学研究作了新的探讨,给出了建立含闭链机构机器人动力学方程的一般方法。旨在把含闭链机构机器人分解成相应的开链机构进行研究,因而大大简化了推导过程。文中通过一个实际工业机器人动力学方程的推导,证实了该方法的可行性。     

Preparation,Growth Mechanisms and Characterizations of ZnSe Films via the Solvothermal Method

With diethylamine as a solvent, ZnSe films were formed on the Si substrate directly from zinc and selenium through the modified solvothermal method. The effects of holding temperature, deposition time and substrate surface treatment on the quality and morpholo-gies of the ZnSe films were investigated. The growth mechanism of ZnSe films was proved to be a layer-nucleation growth process, which was tied in with the Stranski-Krastanov (SK) model. ZnSe films were identified by the X-ray diffraction pattern (XRD), the scan-ning electron microscope (SEM), the X-ray photoelectron spectroscope (XPS) and the photoluminescence (PL) techniques. The results indicate that the modified solvothermal method with diethylamine as a solvent is suitable to prepare high quality ZnSe films.