Precessing motion in stratified radial swirl flow

Vortex/flame interaction is an important mechanism for unsteady combustion in a swirl combustion system. Technology of low emission stirred swirl(Te LESS), which is characterized with stratified swirl flow, has been developed in Beihang University to reduce NOXemission. However,large-scale flow structure would be induced in strong swirl flow. Experiments and computational fluid dynamics(CFD) simulation were carried out to investigate the unsteady flow feature and its mechanism in Te LESS combustor. Hotwire was firstly applied to testing the unsteady flow feature and a distinct mode with 2244 Hz oscillation frequency occurred at the pilot swirl outlet.The flow mode amplitude decayed convectively. Large eddy simulation(LES) was then applied to predicting this flow mode and know about its mechanism. The deviation of mode prediction compared with hotwire test was 0.8%. The spiral isobaric structure in pilot flow passage indicates that precessing vortex core(PVC) existed. The velocity spectrum and phase lag analysis suggest that the periodic movement at the pilot outlet was dominated by precessing movement. Negative tangential momentum gradient reflects that the swirl flow was unstable. Another phenomenon was found out that the PVC movement was intermittently rotated along the symmetric axis.     

大型结构高次曲面外形精密测量技术研究与应用

为了完成对大型结构高次外形曲面高精度测量工作,采用激光扫描与视觉手持测量相结合的方式对结构曲面进行全轮廓点云数据提取。给出了数据融合方案,完成了测量系统搭建。将飞行器理论曲面作为基准面型与测量结果进行轮廓偏差比对,对测量结果进行分析表明该技术可用于大型结构高次曲面外形精密测量。     

航空发动机叶片大曲率型面测量方法研究

大扭角、大曲率等复杂空间曲面叶型是航空发动机叶片发展的趋势,而传统的测量方法已经不能满足这种新型叶片的测量需要。多次的测量比对数据显示,利用CAD模型引导测量并评价的方法不但降低了叶片测量在等高方面的要求,而且消除了投影计算方法中带来的计算误差,更加快速、准确地反映了叶片的真实加工质量。     

大型数控龙门桥式加工中心的研制

针对船舶、航空、轨道交通、核电等行业的大型零件加工需求,研制了大型数控龙门桥式加工中心,3个移动轴行程为3m×5m×0.8m,可实现O.02mm的镗铣加工精度.通过对加工中心若干技术研究集成,使之具备以下重大特点:(1)研究伺服电机解耦控制方法及双驱动同步技术,保证横梁在两侧桥式立柱导轨上的精确同步纵向移动;(2)通过旋转螺母丝杠结构分别独立驱动双主轴头在横梁上的横向移动,实现双主轴独立加工;(3)利用双回转摆动铣头附件及控制系统集成,实现大型零件的五轴数控加工.所研制的加工中心具有工作台承重大、加工效率高、使用方便、自动化程度较高等特点,已成功用于生产.     

空间遥感器大口径反射镜支撑结构型式综述

文章针对空间遥感器大口径反射镜（口径大于500mm）总结了影响支撑结构设计的主要因素，介绍了几种主要的支撑结构型式，并讨论了支撑结构设计中所需要考虑的若干问题。     

基于IMM理论的大型舰船被动定位算法研究

针对相控阵导引头跟踪航母等大型舰船目标的要求,为了给雷达成像进行运动补偿、给目标识别提供更多的先验信息,必须对目标运动参数进行准确的估计,但是常规被动定位算法通常采用单一目标运动模型,难以适应大型军舰运动规律的多样化,导致模型不匹配,使得误差较大,难以对目标参数进行准确估计,为解决上述问题,提出了一种基于交互式多模型(IMM)理论的大型舰船被动定位方法,使用不同的模型来匹配舰船不同的运动状态。仿真结果表明,提出的方法与常规的被动定位算法相比,定位精度明显提高,且易于工程实现。     

双光束补偿扫描系统

提出一种新的高精度大型平面扫描仪。利用双光束补偿系统，扫描头由一特殊光路组成。当入射光通过此光路后，产生对称输出的两束光。当入射光发生角漂或扫描头发生摆动时，输出的两束光对称上下漂移，其中心线保持不变，故扫描形成的基准面保持不变，从而大大提高了测量精度。经实验证明，测量精度优于2．5×10－6。     

Two-level optimization approach for Mars orbital long-duration,large non-coplanar rendezvous phasing maneuvers

A relative dynamics equation-set based on orbital element differences with J₂ effects is derived, based on which a two-level approach is proposed to optimize the Mars orbital rendezvous phasing with a large difference in the initial ascending node. The up-level problem uses the revolution deviation between the target spacecraft and the chaser as the design variable, and employs a linear search to find the optimum. The low-level problem uses the maneuver revolutions, locations, and impulses as the design variables, and is solved using a hybrid genetic algorithm combined with sequential quadratic programming. To improve the solution accuracy, an iteration method is developed to satisfy the terminal constraints of the absolute numerical integration trajectory. Test cases involving Mars sample return missions with large initial node differences are presented, which show that the relative dynamics, two-level optimization model, and hybrid optimization algorithm are efficient and robust. Compared with previously published results, the total velocity increment has been further reduced by utilizing this proposed approach. It is found that a five-impulse plan requires the least quantity of propellant, and a propellant-optimal minimum rendezvous duration exists for this long-duration, large non-coplanar rendezvous problem.     

Damage assessment of large space structures through the variational approach

The present investigation is focused on the solution of a dynamic inverse problem which is concerned with the assessment of damage in large space structures by means of measured vibration data. This inverse problem has been presented as an optimization problem and has been solved through the use of the conjugate gradient method with the adjoint equation, also called the variational approach. When a high number of damaged elements has to be found and these elements are also severely damaged, it is shown that the use of an additional method is necessary in order to provide a better initial guess for the conjugate gradient method. A stochastic method, represented by the genetic algorithm method, has been chosen because it provides robust search in complex spaces and also reduces the chance of converging to local optima. The application of this hybrid approach showed that better results can be achieved, although the computational time for the application analyzed here could increase. The damage estimation has been evaluated using noiseless and noisy synthetic experimental data, and the reported results are concerned with a space truss structure.     

A preliminary Chandra X-ray spectroscopy of the supernova remnant N132D

We present the preliminary results of a Chandra X-ray study of N132D, a young shell-like supernova remnant (SNR) in the Large Magellanic Cloud. The equivalent width maps of emissions from O, Ne, Mg, Si, and S are provided. Spatially resolved spectral analysis for the small-scale regions were tentatively performed. X-ray spectra of the interior can be described with a single-thermal model. The faint interior regions have lower density, higher temperature above 1 keV than that of bright interior regions. The X-ray spectra along the shell can be phenomenally fitted with either a double-vpshock model or a vpshock + powerlaw model. If the non-thermal component is true, N132D would be listed as another X-ray synchrotron SNR.