叶根倒角模拟件设计

为了避免涡轮叶片叶根倒角低周疲劳开裂故障的发生,需借助叶根倒角特征模拟件对叶根低周疲劳强度进行考核。基于几何等效相似和载荷工况等效原则,设计了一种真实叶根倒角的特征模拟件。特征模拟件的榫头/叶身沿着周向投影宽度比例、缘板外侧与榫头外侧距离、缘板厚度、倒角半径等重要几何参数均与真实叶片一致。基于线弹性本构,采用Abaqus软件计算了特征模拟件在等效载荷工况下的应力分布。计算结果表明,特征模拟件的最大应力为187.6 MPa,出现在凸台过渡区倒角处,最危险点第一主应力方向为l₁=0.1141、m₁=0.9873、n₁=-0.1103,均与真实叶片对应部位的应力情况吻合,说明该叶根倒角特征模拟件设计合理,可用于考核真实涡轮叶片倒角的低周疲劳强度。     

模拟载人探月中航天员空间辐射风险评估

空间辐射是长期载人航天飞行任务中影响航天员健康的重要风险因素。为了探求载人探月过程中对空间辐射的合理防护方式,文章借助空间辐射场模型对"嫦娥三号"飞行任务在不同质量厚度材料屏蔽下的舱内空间辐射环境进行了仿真计算,并确定了航天员各器官接受的空间辐射剂量、剂量当量以及有效剂量等辐射防护量以进行辐射风险评估。结果表明,随着屏蔽厚度的增加,航天员的各组织或器官的吸收剂量和剂量当量以及有效剂量均明显降低;采用质量屏蔽的方法对低于100 Me V的质子具有很好的防护效果,但对高能质子或重离子的防护效果不明显。计算和分析显示,载人探月过程中,只要采取适当的防护措施,航天员的空间辐射风险是可控的。     

某涡轴发动机涡轮叶片尾缘孔的蠕变-疲劳寿命预测方法

针对某涡轴发动机的涡轮叶片,建立了考虑应力松弛的蠕变-疲劳寿命分析方法。通过在黏塑性理论框架内耦合蠕变损伤,对某高温合金的非线性蠕变变形进行了数值模拟。结果表明:基于对某涡轮叶片的弹塑性-蠕变分析研究,明确了叶片上前缘和尾缘等关键部位的蠕变损伤及其演化规律,也为确定叶片上的局部危险点提供了一种方法。该模型针对弹塑性应力应变曲线计算误差小于5%,而针对蠕变曲线的模拟精度则处于材料蠕变变形固有属性分散范围内。借助于线性损伤累积寿命理论,分析得到了某涡轮叶片尾缘孔局部考虑了应力松弛的蠕变-疲劳寿命,从而为叶片寿命评价提供了更为合理、工程化应用更好的方法。      

基于LSTM的飞行数据挖掘模型构建方法

提出了一种基于LSTM （Long Short Time Memory）模型的飞行历史数据挖掘模型的构建方法,此模型可以将飞行数据中有价值的目标数据自动提取出来。首先,通过滑动窗口法获得待检测数据;然后,将预先做好的训练样本数据输入到所构造的LSTM模型中进行训练,得到数据挖掘模型;最后,将待检测数据导入到训练好的LSTM模型中进行模式识别,将目标数据片段挖掘出来。结果表明,基于LSTM模型的飞行数据挖掘模型构建方法通用化程度高,可用于挖掘不同类型的目标数据,且识别率高,具有很高的工程应用价值。     

基于局部均值分解和峭度图的滚动轴承包络分析方法

提出了基于局部均值分解(local mean decomposition,LMD)和峭度图(kurtogram)的滚动轴承包络分析方法.该方法中,原始滚动轴承故障振动信号通过LMD进行自适应的频率成分分离和初步降噪,包络分析中带通滤波器的参数通过峭度图客观地提供,从而提高滚动轴承包络分析的准确度.通过对滚动轴承仿真信号以及实验信号的分析,结果表明:在低信噪比情况下,LMD可以自适应分离出滚动轴承的固有振动成分,峭度图可以自动确定包络分析中带通滤波器的参数,与传统包络分析比较,所提方法能更加清晰准确地提取滚动轴承的故障特征.      

酒石酸钠体系中TC18钛合金阳极氧化膜的制备、表征与疲劳性能

在以酒石酸钠为成膜剂的新型无氟环保电解液体系中对TC18钛合金进行阳极氧化,制备出一种钛合金阳极氧化膜。通过扫描电子显微镜和拉曼光谱仪分析了阳极氧化膜的形貌和相结构。采用电化学方法研究了阳极氧化后TC18钛合金的耐腐蚀性能。采用万能高频疲劳试验机进行高频疲劳试验。结果表明：膜层具有沟壑与鼓包的表面形貌。膜层具有非晶态、锐钛矿型及金红石型TiO₂结构,可能有板钛矿TiO₂结构。阳极氧化后TC18钛合金的耐蚀性有显著的提高。阳极氧化后TC18钛合金的拉伸性能与疲劳性能基本不降低,相比于传统硫酸-磷酸型阳极氧化,拉伸性能和疲劳性能得到了一定的改善。     

Cosmic Ray Energetics And Mass for the International Space Station (ISS-CREAM)

The Cosmic Ray Energetics And Mass (CREAM) instrument is configured with a suite of particle detectors to measure TeV cosmic-ray elemental spectra from protons to iron nuclei over a wide energy range. The goal is to extend direct measurements of cosmic-ray composition to the highest energies practical, and thereby have enough overlap with ground based indirect measurements to answer questions on cosmic-ray origin, acceleration and propagation. The balloon-borne CREAM was flown successfully for about 161 days in six flights over Antarctica to measure elemental spectra of Z = 1–26 nuclei over the energy range 10¹⁰ to >10¹⁴ eV. Transforming the balloon instrument into ISS-CREAM involves identification and replacement of components that would be at risk in the International Space Station (ISS) environment, in addition to assessing safety and mission assurance concerns. The transformation process includes rigorous testing of components to reduce risks and increase survivability on the launch vehicle and operations on the ISS without negatively impacting the heritage of the successful CREAM design. The project status, including results from the ongoing analysis of existing data and, particularly, plans to increase the exposure factor by another order of magnitude utilizing the International Space Station are presented.     

Comprehensive data reduction package for the Immersion GRating INfrared Spectrograph: IGRINS

We present a Python-based data reduction pipeline package (PLP) for the Immersion GRating INfrared Spectrograph (IGRINS), an instrument that covers the complete H- and K-bands in one exposure with a spectral resolving power of 40,000. The reduction steps carried out by the PLP include flat-fielding, background removal, order extraction, distortion correction, wavelength calibration, and telluric correction using spectra of A type standard stars. As the spectrograph has no moving parts, the PLP automatically reduces the data using predefined functions for the processes of order extraction, distortion correction, and wavelength calibration. Before the telluric correction of the target spectra, the intrinsic hydrogen absorption features of the standard A star are removed with a Gaussian fitting algorithm. The final result is the flux of the target as a function of wavelength. Users can customize the predefined functions for the extraction of the spectrum from the echellogram and adjust the parameters for the fitting functions for the spectra of celestial objects, using “fine-tuning” options, as necessary. Presently, the PLP produces the best results for point-source targets.     

虚警影响下的备件库存优化

在虚警存在时完好的零部件被误诊为故障件而对维修站点发出备件需求,从而会对备件的需求率高估,所以需要引入虚警率修正备件需求率使之更为精确.证明了当虚警率服从指数分布时,考虑虚警的外场故障发生数仍然符合泊松分布.根据多层可修件库存控制理论,建立考虑虚警率的需求数和期望备件短缺数（EBO,Expected BackOrder）的函数关系,以期望备件短缺数为优化目标,对目标函数进行凸分析,建立面向系统虚警的备件配置凸优化算法,保证所选库存方案在系统发生虚警的情况下提高系统效能,并构建了某型飞机的应用验证案例,给出了最优的备件配置方案.