Ti6Al4V合金微弧氧化陶瓷膜的组织结构研究

采用微弧氧化技术在钛合金表面成功制备出膜厚约100μm的致密陶瓷膜以提高钛合金的耐磨性.SEM结果表明,陶瓷膜完整连续,与基体呈犬牙状牢固结合.XRD衍射结果表明:陶瓷膜主要由金红石型二氧化钛和Al2TiO4晶体相组成.显微硬度结果表明钛合金微弧氧化陶瓷膜的显微硬度为862HV而基体合金硬度仅为412HV,陶瓷膜的硬度远远高于基体合金的显微硬度.摩擦磨损试验表明,镀膜的钛合金磨损量远小于不镀膜钛合金的磨损量,陶瓷膜能提高基体的摩擦磨损性能.     

航空发动机滑油综合监控中的磨损故障融合诊断研究

单一的滑油光谱监控手段容易漏报航空发动机磨损故障.根据滑油光谱监控和自动磨粒检测互补的特点,在某型航空发动机上实施滑油综合监控,应用Dempster-Shafer(D-S)证据理论实现发动机磨损故障的融合诊断,并开发出基于上述监控方法和信息融合诊断的滑油监控专家系统.通过对实际诊断案例进行分析,结果表明:提出的滑油综合监控和融合诊断方法可有效解决该型发动机轴承故障预报的难题.      

Fe/O Ratios in Interplanetary Shock Accelerated Particles

It is widely accepted that diffusive shock acceleration is an important process in the heliosphere, in particular in producing the energetic particles associated with interplanetary shocks driven by coronal mass ejections. In its simplest formulation shock acceleration is expected to accelerate ions with higher mass to charge ratios less efficiently than those with lower mass to charge. Thus it is anticipated that the Fe/O ratio in shock-accelerated ion populations will decrease with increasing energy above some energy. We examine the circumstances of five interplanetary shocks that have been reported to have associated populations in which Fe/O increases with increasing energy. In each event, the situation is complex, with particle contributions from other sources in addition to the shock. Furthermore, we show that the Fe/O ratio in shock-accelerated ions can decrease even when the shock is traveling through an Fe-rich ambient ion population. Thus, although shock acceleration of an Fe-rich suprathermal population has been proposed to explain large Fe-rich solar particle events, we find no support for this proposal in these observations.     

Solar Sources of Heliospheric Energetic Electron Events—Shocks or Flares?

Electrons with near-relativistic (E≳30 keV, NrR) and relativistic (E≳0.3 MeV) energies are often observed as discrete events in the inner heliosphere following solar transient activity. Several acceleration mechanisms have been proposed for the production of those electrons. One candidate is acceleration at MHD shocks driven by coronal mass ejections (CMEs) with speeds ≳1000 km s⁻¹. Many NrR electron events are temporally associated only with flares while others are associated with flares as well as with CMEs or with radio type II shock waves. Since CME onsets and associated flares are roughly simultaneous, distinguishing the sources of electron events is a serious challenge. On a phenomenological basis two classes of solar electron events were known several decades ago, but recent observations have presented a more complex picture. We review early and recent observational results to deduce different electron event classes and their viable acceleration mechanisms, defined broadly as shocks versus flares. The NrR and relativistic electrons are treated separately. Topics covered are: solar electron injection delays from flare impulsive phases; comparisons of electron intensities and spectra with flares, CMEs and accompanying solar energetic proton (SEP) events; multiple spacecraft observations; two-phase electron events; coronal flares; shock-associated (SA) events; electron spectral invariance; and solar electron intensity size distributions. This evidence suggests that CME-driven shocks are statistically the dominant acceleration mechanism of relativistic events, but most NrR electron events result from flares. Determining the solar origin of a given NrR or relativistic electron event remains a difficult proposition, and suggestions for future work are given.     

基于接触状态的叶冠预扭设计

针对某工程的实际问题,建立了叶片三维分析模型,应用谐波平衡法和时频转换法,分析了叶冠结构参数与安装状态下叶冠力学性能的关系,总结了叶冠几何参数对接触状态的影响规律;就叶冠接触状态与叶冠磨损之间的关系进行了讨论;基于接触状态的设计理论,提出了叶冠预扭设计基本思想和工程方法.     

TC4-DT钛合金磨削表面特性及其摩擦磨损性能

钛合金是一种典型难磨削加工材料,磨削表面易出现烧伤、裂纹等热损伤。本文开展了TC4-DT钛合金磨削实验,通过扫描电镜（SEM）、能谱（EDS）、X射线衍射（XRD）、显微硬度仪、金相显微镜及球-盘摩擦磨损实验仪研究了其表面特性及摩擦磨损性能。结果表明：低速磨削表面质量好,摩擦磨损性能较基体略提高;当砂轮线速度为80 m/s时,磨削表面质量良好,摩擦系数为0.38,较基体降低40%;而砂轮线速度为100 m/s时,磨削表面出现严重烧伤、网状裂纹。因此选择合理的高速磨削工艺可避免烧伤、裂纹等热损伤缺陷,并可有效改善表面摩擦磨损性能;磨削表面干摩擦磨损机制为磨粒磨损、粘着磨损和剥层磨损。     

GH4169合金反挤压成形模具磨损

基于修正 Archard 磨损模型,采用数值模拟方法系统分析了 GH4169合金反挤压成形过程中各挤压工艺参数对模具磨损的影响规律。结果表明：在选取的参数范围内,挤压凸模最易产生磨损失效的区域为凸模圆角处,模具最大磨损深度随凸模圆角半径及坯料预热温度的增大而降低,随摩擦系数的增大而增大;当挤压速率小于100 mm ／s时,模具最大磨损深度随挤压速率的增大而减小,当挤压速率大于100mm ／s 时,模具最大磨损深度随挤压速率的增大先增大后减小。最佳工艺参数坯料预热温度1020℃,摩擦系数0．05,变形速率100mm ／s,模具预热温度300℃时模具磨损量最小,为9．28×10－3 mm。     

小型回流燃烧室多工况碳黑分布预测

为了研究小型回流燃烧室不同条件下的工作状态,并分析其产生积碳现象的原因,采用k-ε湍流模型、EDC湍流燃烧等模型对该燃烧室多个工况进行数值计算。结果表明,燃烧室性能参数计算值与台架数据较吻合,各个状态下参数相对误差均小于1.37%。根据各工况的温度分布的变化,发现燃烧室火焰随工况降低逐渐向火焰筒头部收缩。计算了各工况蒸发管内的燃油蒸发率,发现蒸发率在低工况时明显降低。根据出口温度分布情况,计算出口温度分布系数OTDF为0.35。分析碳黑粒子的分布,发现积碳现象主要在火焰筒头部,其原因主要是燃烧不充分和冷却气膜的缺失。     

C/C素坯密度对GSIC/C-SiC复合材料摩擦磨损性能的影响

采用气相渗硅工艺(GSI)制备C/C-Si C复合材料,研究了C/C素坯密度对GSI C/C-Si C复合材料物相组成与摩擦磨损性能的影响,分析了C/C-Si C复合材料的制动过程,并归纳了其摩擦磨损机理。结果表明,随着C/C素坯密度的增大,GSI C/C-Si C复合材料的密度呈递减趋势,且C含量和开气孔率逐渐增加,而Si C含量和残余Si含量逐渐减少;自对偶条件下,复合材料的平均摩擦系数、磨损率均呈现先增大后减小的趋势,当C/C素坯密度为1.25g/cm3时有最大值,而制动稳定系数则不断增大。GSI C/C-Si C复合材料的制动过程是犁沟效应和粘着效应共同作用的结果,制动初始阶段和刹停阶段以犁沟效应为主,中间阶段以粘着效应为主。     

GT35硬质合金材料高温摩擦磨损特性研究

利用球-盘高温摩擦磨损试验机对GT35硬质合金进行摩擦磨损实验,研究了GT35硬质合金材料的摩擦磨损特性及机理。分析了不同温度和不同摩擦半径情况下GT35硬质合金的摩擦磨损行为。结果表明:在法向载荷不变的条件下,GT35硬质合金的摩擦系数和比磨损率均随温度的上升而增大,其摩擦系数和比磨损率随摩擦半径的增加也呈上升的变化趋势。