基于光场成像的快照式气膜孔三维测量技术

叶片气膜孔的几何参数对其冷却效率具有十分重要的影响，需采取有效手段对加工的气膜孔几何参数进行检测。基于光场成像原理，初步探索了单光场相机快照式三维测量技术在气膜孔检测上的应用。与其他光学测量技术相比，该技术仅通过一次拍摄，即可快速从捕获的单张原始光场图像中计算得到气膜孔的三维点云数据，其数据采集效率很高。实验中对一组标准量块进行了测量，展示了单光场相机应用于工业级精密测量的潜力。对实际叶片上气膜孔几何参数的检测结果初步表明了该技术应用于气膜孔三维测量的可能性。由于单光场相机成像系统的结构简单，易于操作且便于与其他传感器设备集成，可为气膜孔三维测量问题提供一种新的解决方案。     

几何尺寸约束的超燃冲压发动机推力喷管设计

针对机体/推进系统一体化要求，提出了一种几何尺寸约束的超燃冲压发动机推力喷管设计方法，以实现在满足几何约束条件下优化喷管的气动性能。采用数值模拟对提出的设计方法展开了研究，在此过程中，首先校核了数值方法有效性并确定了网格分辨率。进一步就喷管设计过程中2个关键设计因子——比例因子和非对称因子开展了影响研究。最后为验证本文提出的设计方法的有效性和优越性，将其与典型截短设计方法进行对比分析。结果表明，相比截短方法，本文提出的设计方法不仅能够获得满足几何约束的喷管，同时可使喷管推力系数、升力和俯仰力矩分别提升33.36%、265.75%和37.21%。此外，本文提出的设计方法还可以通过调整设计因子来获得不同气动性能的喷管，进而满足应用过程中的实际需求。     

Laser-induced oxidation assisted micro milling of high aspect ratio microgroove on WC-Co cemented carbide

Severe tool wear and poor surface quality are the main problems during micro machining of cemented carbide. In this work, an innovative hybrid process of laser-induced oxidation assisted micro milling (LOMM) was proposed to solve the problems. A nanosecond laser was utilized to induce oxidation of the WC-20%Co material, producing loose oxide which was easy to remove. The micro machinability of the material was improved by laser-induced oxidation. The oxidation mechanisms of cemented carbide were studied. A microgroove with a depth of 2.5 mm and aspect ratio of 5 was fabricated successfully. The milling force, surface quality and tool wear mechanisms were investigated. For comparison, a microgroove was also fabricated with conventional micro milling (COMM) using identical milling parameters. Results revealed that in LOMM the milling force and tool wear rate were extremely low during removing the oxide. The machined surface quality and dimensional accuracy achieved by LOMM were superior to those obtained by COMM. The surface roughness S_a of the microgroove bottom reached 88 nm in LOMM, while the cross-sectional geometry of the microgroove was a trapezoid. Perpendicularity of the microgroove sidewall machined by LOMM was better than that by COMM. The tool wear forms in LOMM were coating spalling and slight tool nose breakage. Compared with COMM, the tool life in LOMM was prolonged significantly. It indicates that the proposed hybrid process is an effective and efficient way to fabricate high aspect ratio micro-features with high dimensional accuracy.     

改进BA优化的MKSVDD航空发动机工作状态识别

为了提高航空发动机工作状态识别准确率和效率，避免人工识别中存在的误判和耗时耗力问题，提出了基于混沌脉冲蝙蝠算法（CRBA）优化的多核支持向量数据描述（CRBA-MKSVDD）智能识别方法。研究了多核支持向量数据描述（MKSVDD）改进策略，引入混沌脉冲发射率提高了蝙蝠算法（BA）的收敛速度和收敛精度，得到了CRBA；通过CRBA优化MKSVDD的惩罚因子和核参数，同时对飞参数据进行了特征提取；基于特征飞参数据训练了CRBA-MKSVDD分类器，并对某型发动机一个飞行架次的工作状态进行了识别。结果表明，该方法识别准确率达到97.547 9%，可用于与发动机工作状态的相关研究和应用。     

A progressive approach to predict shot peening process parameters for forming integral panel of Al7050-T7451

In this paper, a progressive approach to predict the multiple shot peening process parameters for complex integral panel is proposed. Firstly, the invariable parameters in the forming process including shot size, mass flow, peening distance and peening angle are determined according to the empirical and machine type. Then, the optimal value of air pressure for the whole shot peening is selected by the experimental data. Finally, the feeding speed for every shot peening path is predicted by regression equation. The integral panel part with thickness from 2 mm to 5 mm and curvature radius from 3200 mm to 16000 mm is taken as a research object, and four experiments are conducted. In order to design specimens for acquiring the forming data, one experiment is conducted to compare the curvature radius of the plate and stringer-structural specimens, which were peened along the middle of the two stringers. The most striking finding of this experiment is that the outer shape error range is below 3.9%, so the plate specimens can be used in predicting feeding speed of the integral panel. The second experiment is performed and results show that when the coverage reaches the limit of 80%, the minimum feeding speed is 50 mm/s. By this feeding speed, the forming curvature radius of the specimens with different thickness from the third experiment is measured and compared with the research object, and the optimal air pressure is 0.15 MPa. Then, the plate specimens with thickness from 2 mm to 5 mm are peened in the fourth experiment, and the measured curvature radius data are used to calculate the feeding speed of different shot peening path by regressive analysis method. The algorithm is validated by forming a test part and the average deviation is 0.496 mm. It is shown that the approach can realize the forming of the integral panel precisely.     

基于改进粒子群优化模糊控制的MPPT算法研究

在光照强度和温度变化时,常规的最大功率点跟踪(MPPT)算法难以快速准确地跟踪光伏系统最大功率点。针对此问题,设计了一种改进粒子群优化算法(PSO)的模糊控制器。首先,依据常规MPPT特性,设计了一种带调整因子的模糊控制算法以快速收敛到最大功率点；然后,采用参数自适应PSO对设计的模糊控制器调整因子进行动态优化。仿真结果表明:所设计的参数自适应PSO优化模糊控制器能快速准确地跟踪最大功率点,保证了MPPT的动态响应速度和稳态精度,提高了光伏系统的工作效率。     

蜻蜓起飞过程飞行特征实验

针对蜻蜓自由起飞过程和准自由起飞过程进行实验观测,采用两个光轴相互垂直的高速摄像机进行拍摄,通过特征点匹配和三维重构方法准确地捕捉了两种起飞过程中蜻蜓身体和翅膀的运动参数,并进行运动特征分析与对比。实验结果表明:蜻蜓在自由起飞过程中采用同步振翅,离地后逐步转换成异步振翅(约110°),最大瞬时竖直加速度可以达到20m/s2;在准自由起飞过程中采用异步振翅(相位差180°),之后相位差逐步降低,最大瞬时竖直加速度为12m/s2;此外发现同步振翅、大攻角下拍及大拍动角有利于升力的产生。      

Inverse identification of constitutive parameters of Ti2AlNb intermetallic alloys based on cooperative particle swarm optimization

Ti₂AlNb intermetallic alloy is a relatively newly developed high-temperature-resistant structural material, which is expected to replace nickel-based super alloys for thermally and mechanically stressed components in aeronautic and automotive engines due to its excellent mechanical properties and high strength retention at elevated temperature. The aim of this work is to present a fast and reliable methodology of inverse identification of constitutive model parameters directly from cutting experiments. FE-machining simulations implemented with a modified Johnson-Cook (TANH) constitutive model are performed to establish the robust link between observables and constitutive parameters. A series of orthogonal cutting experiments with varied cutting parameters is carried out to allow an exact comparison to the 2D FE-simulations. A cooperative particle swarm optimization algorithm is developed and implemented into the Matlab programs to identify the enormous constitutive parameters. Results show that the simulation observables (i.e., cutting forces, chip morphologies, cutting temperature) implemented with the identified optimal material constants have high consistency with those obtained from experiments, which illustrates that the FE-machining models using the identified parameters obtained from the proposed methodology could be predicted in a close agreement to the experiments. Considering the wide range of the applied unknown parameters number, the proposed inverse methodology of identifying constitutive equations shows excellent prospect, and it can be used for other newly developed metal materials.     

Quasars and their emission lines as cosmological probes

Quasars are the most luminous sources in the Universe. They are currently observed out to redshift z≈7$z\approx 7$ when the Universe was less than one tenth of its present age. Since their discovery 50 years ago astronomers have dreamed of using them as standard candles. Unfortunately quasars cover a very large range (8 dex) of luminosity making them far from standard. We briefly review several methods that can potentially exploit quasars properties and allow us to obtain useful constraints on principal cosmological parameters. Using our 4D Eigenvector 1 formalism we have found a way to effectively isolate quasars radiating near the Eddington limit. If the Eddington ratio is known, under several assumptions it is possible to derive distance independent luminosities. We discuss the main statistical and systematic errors involved, and whether these “standard Eddington candles” can be actually used to constrain cosmological models.     

The effective temperatures of O-type stars from UV spectroscopy

We present an analysis of high resolution spectra in the far-UV – UV range (∼905–2000 Å) with non-LTE, spherical, hydrodynamical, line-blanketed models, of three O-type Galactic stars, and derive their photospheric and wind parameters. These data extend previously analyzed samples and fill a gap in spectral type coverage. The combined sample confirms a revised (downward) T_eff scale with respect to canonical calibrations, as found in our previous works from UV and optical spectra, and in recent works by other authors.