跨音速翼型风洞的洞壁干扰研究

利用三个几何相似的 RAE104翼型模型,用实验方法确定西工大翼型风洞(TAWX)的无堵塞干扰开闭比。对于不带测压轨及带测压轨两种状态的开槽壁分别采用2%及4%开闭比可认为近似于无堵塞干扰。利用测压轨测量该翼型风洞上下壁附近控制面的静压分布,并利用快速富里叶变换法计算马赫数及迎角修正量。由 TAWX 风洞与西德 DFVLR TWB 风洞实验结果的比较可以看出,当迎角为零时,两者结果吻合较好,说明无堵塞干扰开闭比的确定基本上是正确的,经过快速富里叶变换法进行马赫数及迎角修正后的 TAWX 有升力的实验结果也与 TWB 结果接近。     

高温天线罩材料研究进展

对目前主要几种高温天线罩材料体系，包括氧化铝陶瓷、石英陶瓷、微晶玻璃、纤维增强二氧化硅基复合材料、纤维增强磷酸盐基复合材料以及硅氧氮陶瓷材料的研究发展和应用情况进行了简要的综述。     

反馈线性化飞行控制的应用问题研究

分析了反馈线性化飞行控制的奇异摄动降阶条件,讨论了外环解耦矩阵的奇异域和跟踪误差,建立了操纵面冗余时分配偏转指令的原则。用过失速转弯等机动进行了数值仿真验证。     

航空发动机燃油与控制系统的研究与展望

归纳和分析了国内外军用航空发动机燃油与控制系统的研制现状和今后的发展方向 ,简要介绍和评述了主燃油控制、加力燃油控制、尾喷口控制、防喘控制、发动机状态监视 ,特别是FADEC系统的技术特点、方案选择和研究动向。从中可以看出 ,这些方面的技术进步推动了航空发动机的发展     

离心加速声中液态浸渗纤维预制体动力学分析

在将纤维预制体视为“毛细管束”的基础上,采用达西定律建立了离心加速场中金属液浸渗纤维预制体的浸渗动力学模型。采用该模型分析了离心加速场中金属液浸渗纤维预制体的临界转速,考察了金属液浅注量、设备转速、铸件高度、金属液原如外半径以及纤维预制体孔隙率对离心加速场中金属 浸润纤维预制体的影响。结果表明,金属液浸润纤维预制体的临界转速只与临界压力、金属液的浇注量、铸件高度以及纤维预制休性质有关;增加金属液浇注量、设备转速及金属液原始外半径,降低铸件高度、预制体纤维体积分数,有利于金属液的浸渗。     

液压余度舵机同步传动研究

几个舵机驱动同一控制对象,通道间产生力的纷争,本文采用均衡网络来减轻力的纷争,而均衡网络的参数则根据解耦控制理论导出。实际系统的实验证明本文所提出的消除余度通道间力纷争保证同步传动的方案是有效的。文章给出了最优均衡网络的参数设计公式。     

破坏性物理分析(DPA)在高可靠半导体器件质量验证中的作用

文章介绍了破坏性物理分析(DPA)内容,以及它在高可靠性半导体器件质量验证中的作用。通过大量的数据表明,DPA 能有效地评价半导体器件的批质量.     

The Seed Population for Energetic Particles Accelerated by CME-Driven Shocks

Understanding properties of solar energetic particle (SEP) events associated with coronal mass ejections has been identified as a key problem in solar-terrestrial physics. Although recent CME shock acceleration models are highly promising, detailed agreement between theoretical predictions and observations has remained elusive. Recent observations from ACE have shown substantial enrichments in the abundances of ³He and He⁺ ions which are extremely rare in the thermal solar wind plasma. Consequently, these ions act as tracers of their source material, i.e., ³He ions are flare suprathermals and He⁺ ions are interstellar pickup ions. The average heavy ion composition also exhibits unsystematic differences when compared with the solar wind values, but correlates significantly with the ambient suprathermal material abundances. Taken together these results provide compelling evidence that CME-driven shocks draw their source material from the ubiquitous but largely unexplored suprathermal tail rather than from the more abundant solar wind peak. However, the suprathermal energy regime has many more contributors and exhibits much larger variability than the solar wind, and as such needs to be investigated more thoroughly. Answers to fundamental new questions regarding the preferred injection of the suprathermal ions, the spatial and temporal dependence of the various sources, and the causes of their variability and their effects on the SEP properties are needed to improve agreement between the simulations and observations.     

Global Response of Martian Plasma Environment to an Interplanetary Structure: From Ena and Plasma Observations at Mars

As a part of the global plasma environment study of Mars and its response to the solar wind, we have analyzed a peculiar case of the subsolar energetic neutral atom (ENA) jet observed on June 7, 2004 by the Neutral Particle Detector (NPD) on board the Mars Express satellite. The “subsolar ENA jet” is generated by the interaction between the solar wind and the Martian exosphere, and is one of the most intense sources of ENA flux observed in the vicinity of Mars. On June 7, 2004 (orbit 485 of Mars Express), the NPD observed a very intense subsolar ENA jet, which then abruptly decreased within ∼10 sec followed by quasi-periodic (∼1 min) flux variations. Simultaneously, the plasma sensors detected a solar wind structure, which was most likely an interplanetary shock surface. The abrupt decrease of the ENA flux and the quasi-periodic flux variations can be understood in the framework of the global response of the Martian plasma obstacle to the interplanetary shock. The generation region of the subsolar ENA jet was pushed towards the planet by the interplanetary shock; and therefore, Mars Express went out of the ENA jet region. Associated global vibrations of the Martian plasma obstacle may have been the cause of the quasi-periodic flux variations of the ENA flux at the spacecraft location.     

An Introduction to CMEs and Energetic Particles

Energetic particle observations in the interplanetary medium provide fundamental information about the origin, development and structure of coronal mass ejections. This paper reviews the status of our understanding of the ways in which particles are energised at the Sun in association with CMEs. This understanding will remain incomplete until the relationship between CMEs and flares is determined and we know the topology of the associated magnetic fields. The paper also discusses the characteristics of interplanetary CMEs that may be probed using particle observations.