3He-Rich Solar Energetic Particle Events

³He-rich solar energetic particle (SEP) events show huge enrichments of ³He and association with kilovolt electrons and Type-III radio bursts. Observations from a new generation of high resolution instruments launched on the Wind, ACE, Yohkoh, SOHO, TRACE, and RHESSI spacecraft have revealed many new properties of these events: the particle energy spectra are found to be either power-law or curved in shape, with the ³He spectrum often being distinctly different from other species. Ultra-heavy nuclei up to >200 amu are found to be routinely present at average enrichments of >200 times solar-system abundances. The high ionization states previously observed near ∼1 MeV/nucleon have been found to decrease towards normal solar coronal values in these events. The source regions have been identified for many events, and are associated with X-ray jets and EUV flares that are associated with magnetic reconnection sites near active regions. This paper reviews the current experimental picture and theoretical models, with emphasis on the new insights found in the last few years.     

一种用于纳米颗粒场致发射推力器的自中和技术

纳米颗粒场致发射推力器(NFET)是一种用于微小卫星的固体工质静电推力器,为促进NFET的工程研制,提出一种新的自中和技术——反向充电中和策略。为研究这种自中和技术的设计方法,建立相应的数值模型以模拟该中和技术下羽流输运过程,并且,在真空舱中开展NFET的羽流测量试验来验证中和模型的正确性。以比色温度计和"打靶法"装置来分别测量羽流温度分布和推力,通过试验与仿真结果的对比,羽流温度变化的试验结果与仿真结果在定性规律上一致,推力的计算误差在9%～10%。在验证模型正确性的基础上,利用该数值模型对关键设计参数进行数值分析。结果表明:引出极与发射极的内径比变化会导致外加电场对剩余电荷颗粒作负功,引起推力下降,该物理参数在0.94附近时,推力达到极大值;而随着颗粒直径的增加,羽流中和区域整体向下游推移,推力升高。本文结论可为NFET的反向充电中和策略提供设计参考。     

A numerical model for bird strike on sidewall structure of an aircraft nose

In order to examine the potential of using the coupled smooth particles hydrodynamic(SPH) and finite element(FE) method to predict the dynamic responses of aircraft structures in bird strike events, bird-strike tests on the sidewall structure of an aircraft nose are carried out and numerically simulated. The bird is modeled with SPH and described by the Murnaghan equation of state, while the structure is modeled with finite elements. A coupled SPH–FE method is developed to simulate the bird-strike tests and a numerical model is established using a commercial software PAM-CRASH. The bird model shows no signs of instability and correctly modeled the break-up of the bird into particles. Finally the dynamic response such as strains in the skin is simulated and compared with test results, and the simulated deformation and fracture process of the sidewall structure is compared with images recorded by a high speed camera. Good agreement between the simulation results and test data indicates that the coupled SPH–FE method can provide a very powerful tool in predicting the dynamic responses of aircraft structures in events of bird strike.     

The elemental composition in energetic particle events at high heliospheric latitudes

The relative abundances of low energy ions (0.6–2.0 MeV/n) in solar energetic particle (SEP) and corotating interaction region (CIR) events have been measured by the EPAC experiment aboard Ulysses since launch in October 1990 until the present time. We give an overview of the abundances of heavy ions (He, C, Ne, Fe) relative to oxygen during energetic particle events lasting longer than 5 days during the in- and out-of-ecliptic phase of the mission. While the period Oct. 1990 to Aug. 1992 was dominated by high solar activity the Ulysses out of ecliptic passage at solar latitudes up to 45° went parallel to the declining phase of solar activity. Thus a very clear structure of corotating interaction regions was observed. While the in-ecliptic composition is in general agreement with measurements made near the Earth, the development of the CIR-composition shows two phases: From Aug. 1992 to May 1993 the C/O-ratio is 0.55–0.70, afterwards it increases to 0.8–0.9. This increase is correlated to the disappearance of the current sheet at 30° solar latitude reported by Smithet al. (1993).     

发动机磨粒统计分布规律与磨损状态监测研究

根据对 WZ- 6航空发动机等由滑油润滑的机械零件磨损磨粒的显微形态统计研究 ,提出了磨屑尺寸分布的 Weibull分布模型 ,探讨了滑油取样和磨粒采样等随机误差的估计及航空发动机磨损状态监测和故障诊断的方法     

Ti-51.8at%Ni形状记忆合金中Ti_3Ni_4相的析出过程

 用透射电镜系统地研究了Ti-51.8at％Ni形状记忆合金在300～600℃时效时Ti_3Ni_4相的析出过程。结果表明:Ti_3Ni_4相以均匀成核方式从过饱和基体中弥散析出。时效初期,Ti_3Ni_4相为细小颗粒状;随时效时间延长或时效温度升高,Ti_3Ni_4相逐渐长大为透镜片状,最终粗化为粗片状。Ti_3Ni_4相通常与基体保持良好的共格关系,其共格应变场衬度随Ti_3Ni_4相尺寸增大而变化,至Ti_3Ni_4相聚集粗化后,与基体的共格关系逐渐丧失,并在其周围基体中产生位错,位错的柏氏矢量为1/2(111)_(B2)或1/2(111)_(B2)。     

航空发动机吸入颗粒物静电感应特性的模拟实验及分析

利用静电传感器和SC-010型环境试验箱等硬件搭建了吸入颗粒物静电监测模拟实验平台,并在此实验平台上展开了针对航空发动机吸入颗粒物静电感应特性的模拟实验研究,成功获取相应静电监测信号。实验设置颗粒材料、管道流速、颗粒粒径和颗粒投入质量4种变量作为变量条件,分别进行4组单一变量的对比实验,采集在不同颗粒材料、不同管道流速、不同颗粒粒径以及不同颗粒质量浓度环境下带电颗粒所产生的静电感应信号,对每组实验信号的活动率水平(AL)、正/负事件率(PER/NER)和绝对平均幅值等特征参数进行相应的数据分析和对比,并得到了一些有用的结论。实验发现,上述4种变量条件分别对静电感应信号的绝对时域平均幅值、AL参数、PER/NER参数有不同程度的影响。     

基于灰色聚类的磨粒自动识别

 将灰色系统理论中的聚类分析技术用于磨损颗粒的自动识别, 编制了相应的计算机模拟程序。在对磨粒图象的形态特征参数进行敏感性分析的基础上, 确定了各参数的灰类白化权函数, 并结合磨粒识别的试验研究, 给出了磨粒各特征参数的聚类权值。应用此方法对一组标准磨粒进行了模拟识别, 识别正确率在90% 以上, 并且识别速度很快, 大大优于传统的磨粒识别方法。     

模型发动机内凝相颗粒碰撞的数值模拟

针对燃烧室内的高温液态凝相粒子,利用所建立的数学模型对聚集状态下粒子间的碰撞与聚合及其与发动机壳体之间的相互作用过程开展了数值分析,获得了收敛管内壁面上液膜厚度及从出口处逃逸的粒子直径分布,并和实验数据进行了比较分析。结果表明在发动机两相内流场计算中,将凝相粒子看成无蒸发的液滴更为合适;聚集状态下凝相粒子间的碰撞与聚合对粒子直径的分布有很大的影响;粒子和壁面之间的相互碰撞不但会导致大量小尺寸粒子的生成,而且也是收敛管内壁面上金属膜形成的直接原因。     

挤压成型对LC4CS铝合金棒材阳极氧化膜结构的影响

研究了挤压成型对LC4CS铝合金棒材表面阳极氧化膜微观结构的影响。采用金相显微（OM）技术、扫描电镜（SEM）和能谱分析（EDS）等方法分析了铝合金基体中合金相的种类和分布、组织结构的变化规律以及阳极氧化膜的表面及断面形貌。研究发现,试样表面阳极氧化膜的结构特征与基体组织特征具有一致性。基体中的阳极相和阴极相颗粒分别导致了氧化膜中孔洞和夹杂缺陷的产生,在挤压变形中形成的析出相带以及不完全再结晶组织是造成氧化膜中凹坑结构和复杂网纹结构的主要原因。