复合材料与金属胶接结构的次弯曲效应研究

复合材料与金属胶接单搭接的次弯曲效应引起的剥离应力,会大大降低接头的强度。采用有限元方法分析复合材料铺向角、铺层顺序及斜削对次弯曲的影响,并进一步研究分析次弯曲和胶层剥离应力、板的弯曲刚度之间的关系。结果表明：次弯曲影响剥离应力的大小;弯曲刚度越大,次弯曲越小;斜削有助于减小次弯曲。     

燃油射流横流穿透深度试验和数值模拟

采用激光粒子成像测速仪(PIV),试验研究了不同动量比下燃油射流在横向空气流中的穿透深度特性。同时,采用数值计算方法,对射流穿透特性进行了模拟,并将试验和计算结果,分别与已有的经验关系式,及考虑气动韦伯数影响修改后的关系式进行对比。结果表明:燃油射流上边界深度与幂指数关系式较吻合;采用VOF两相流模型能较准确地模拟出燃油射流的喷雾核心深度;修改后的关系式与不同燃油-空气动量比范围下的喷雾核心深度较吻合;燃油-空气动量比和气动韦伯数,是影响燃油射流横流穿透深度的主要参数。     

Type II Solar Radio Bursts: Theory and Space Weather Implications

Recent data and theory for type II solar radio bursts are reviewed, focusing on a recent analytic quantitative theory for interplanetary type II bursts. The theory addresses electron reflection and acceleration at the type II shock, formation of electron beams in the foreshock, and generation of Langmuir waves and the type II radiation there. The theory's predictions as functions of the shock and plasma parameters are summarized and discussed in terms of space weather events. The theory is consistent with available data, has explanations for radio-loud/quiet coronal mass ejections (CMEs) and why type IIs are bursty, and can account for empirical correlations between type IIs, CMEs, and interplanetary disturbances. This revised version was published online in August 2006 with corrections to the Cover Date.     

侧壁有出流孔的通道流场实验研究

用五孔探针对侧壁开有出流孔的通道流场进行了详细测量，着重研究出流孔上、下游截面内的流动规律,分析了错排孔对通道流场的影响。实验发现出流孔上游各截面内的流动沿流向呈加速趋势，其下游截面的流速先急剧减缓，然后逐渐加速直至下一出流。距孔最近的上游截面内气流明显向孔偏转，由于惯性作用，孔下游各截面内的二次流仍很显著。     

梯度热障涂层的设计

 采用电子束物理气相沉积方法 (EB PVD)制备了梯度热障涂层,其结构设计为NiCoCrAlY粘结层 /Al₂O₃ YSZ过渡层 /YSZ陶瓷层。YSZ陶瓷层的结构为柱状晶结构,Al₂O₃ YSZ梯度过渡层为梯度微孔结构。采用有限元方法对梯度热障涂层进行热应力分析,优化了Al₂O₃ YSZ梯度过渡层的组成。计算结果表明,梯度涂层的内应力显著降低,而且界面及其附近应力和应变变化较平缓。过渡层厚度的增加有利于降低涂层内应力和缓和涂层界面处的应力集中。     

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CATIA的机床夹具元件快速造型方法

介绍了基于CATIA的CAA架构对实体进行参数化建模的方法,以一个航空夹具设计为实例,开发了基于CAA及零件特征的参数化航空夹具设计模块,为基于CATIA的航空夹具元件快速造型做了技术方法的探索.     

焊后时效处理对2219铝合金VPTIG接头微区组织和显微硬度的影响

研究了不同温度焊后时效处理对2219铝合金变极性钨极氩弧焊(VPTIG)接头各微区显微组织的影响,采用显微硬度测试和透射电镜观察分析焊接接头各微区析出相的形貌和分布。结果表明,焊后时效处理温度不同,焊接接头各微区显微组织和硬度发生的变化不同。热影响区中的完全回复区对焊后时效最为敏感,低温处理时显微硬度就有明显增长,并在160℃处理时达到最大涨幅;焊缝区变化相对较小,其显微硬度的最高涨幅出现在210℃,且小于前者;热影响区中的过时效区最为稳定,显微硬度的最大增长同样出现在160℃,但涨幅很小。透射电镜观察表明,焊接接头各微区的显微硬度变化主要与时效强化相的析出行为有关。     

LIPS-200离子推力器放电室原初电子动力学行为的数值模拟研究

为了得到试验测量不到的气体放电过程中电磁场作用下单个原初电子的动力学行为,建立了LIPS-200离子推力器放电室二维仿真模型,应用网格粒子法(PIC)和蒙特卡洛碰撞(MCC)模拟法对其进行了研究。模拟得到在额定工况下原初电子和中性原子之间的碰撞概率、原初电子损耗率、电磁场分布对其运动速度及运动轨迹的影响等。结果表明磁铁表面磁感强度最大,越靠近放电室内部磁感强度越小,对称轴区域无磁场分布,原初电子在电磁场作用下沿磁力线作加速螺旋运动;运动等离子体的自洽电势大小范围仅为0~2.0V,几乎不会影响等离子体运动;对应总原初电子个数为1.2×106时直接被阳极表面吸收的损耗率仅为0.02%。     

新型高温/超高温热障涂层及制备技术研究进展

简单介绍了先进航空发动机高温/超高温热障涂层(TBCs)的研究背景、意义和现状;简述了近年来国际上在新一代超高温TBCs方面的研究进展。重点介绍了近年来北京航空航天大学在新型高温/超高温TBCs方面的研究成果,包括新型超高温、高隔热陶瓷隔热层材料,1 150℃以上新型抗高温氧化金属粘结层材料,以及电子束物理气相沉积(EB-PVD)、等离子体激活EB-PVD(PA EB-PVD)和等离子物理气相沉积(PS-PVD)等新型制备工艺。最后对TBCs在未来高性能航空发动机上的应用及发展趋势进行了展望。