粉末烧结法制备Al/Tb0.3Dy0.7Fe1.95磁致伸缩复合材料

采用粉末烧结法制备了Al/Tb0.3Dy0.7Fe1.95磁致伸缩复合材料,研究了烧结温度对烧结体的显微结构、相组成、磁致伸缩、抗压强度等性能的影响.研究结果表明,600 ℃烧结时,烧结体中仍主要存在Al与GMM合金相,烧结获得较理想的相分布状态.随着烧结温度的增加,复合体中非GMM相越来越多,原始相减少.当1200 ℃烧结时,烧结体中主要存在杂相,已几乎没有GMM相.随着烧结温度的增加,复合材料的λs和抗压强度明显下降,烧结温度为600 ℃时,烧结体的λs和抗压强度最大,分别为405×10-6和61.71MPa.其不足是,复合材料仍呈现明显的脆性特征.     

基于神经网络补偿的室内无人机组合导航系统

针对无人飞行器在环境特征突变情况下数据融合的可靠性大幅下降问题，提出了神经网络预测补偿的组合导航算法。首先利用扩展卡尔曼滤波和粒子滤波对激光、光流等传感器得到的数据进行融合，然后采用径向基函数（RBF）神经网络对粒子滤波前后的误差进行预测。当激光数据可靠时，RBF神经网络进行训练学习模式，当激光数据中断或者不可靠时，利用训练后的模型对系统进行误差补偿。利用无人飞行器在室内环境下进行定点和轨迹实验，结果表明补偿后的位置导航信息能够明显降低激光数据不可靠时带来的定位误差。     

考虑机翼尾流影响的运输类飞机后体气动外形优化设计（英文）

在某典型运输机翼身组合体的构型上,进行了考虑机翼尾流影响的机身后体气动外形优化设计研究。基于翼身组合体构型建立了考虑尾流影响和部分工程约束的优化设计系统,并对后体构型在巡航状态下进行了优化设计。以比较适合描述后体变形的NURBS样条基函数为空间控制体属性引入FFD自由变形技术,通过在FFD控制框架对该运输机后体进行了空间属性构建。采用无限差值动网格技术提高空间网格的更新效率并保证网格质量。利用改进Kriging代理模型、量子粒子群优化算法提高优化效率和全局寻优能力。为减小巡航阻力,对某运输机后体的上翘角、截面形状等参数进行了优化设计,优化结果显示,设计后的机身气动特性明显提高。     

XPDM型露点仪在医用氧气分析中的应用

介绍了XPDM型露点仪的工作原理、仪器结构、技术指标、操作方法等.     

喷射沉积Ni3Al基高温合金及其复合材料的显微组织和力学性能

利用喷射沉积技术成功地制备了Ｎｉ－Ａｌ－Ｍｏ系Ｎｉ３Ａｌ基高温合金及其复合材料盘坯，对其显微组织和力学性能进行了测试和分析，并对陶瓷粒子的复合机制进行了初步探讨。     

基于逐次升阶的翼型参数化与气动优化方法研究

研究了基本Bezier样条曲线的特性,对比了不同阶次Bezier曲线对超临界翼型的几何描述能力以及由几何偏差带来的气动性能的偏差。利用Bezier曲线的特性提出逐次升阶的翼型参数化方法,结合改进的粒子群优化算法,建立了逐步扩展设计空间的气动优化设计方法,兼顾设计空间和优化效率,很好地解决了设计质量和设计效率之间的矛盾。最后通过典型翼型的优化设计,对比了文中方法与传统Hicks-Henne型函数方法,验证了文中方法的可行性和高效性。     

Advances in modeling gradual solar energetic particle events

Solar energetic particles pose one of the most serious hazards to space probes, satellites and astronauts. The most intense and largest solar energetic particle events are closely associated with fast coronal mass ejections able to drive interplanetary shock waves as they propagate through interplanetary space. The simulation of these particle events requires knowledge of how particles and shocks propagate through the interplanetary medium, and how shocks accelerate and inject particles into interplanetary space. Several models have appeared in the literature that attempt to model these energetic particle events. Each model presents its own simplifying assumptions in order to tackle the series of complex phenomena occurring during the development of such events. The accuracy of these models depends upon the approximations used to describe the physical processes involved in the events. We review the current models used to describe gradual solar energetic particle events, their advances and shortcomings, and their possible applications to space weather forecasting.     

Solar Energetic Particle Charge States: An Overview

The ionic charge distributions of solar energetic particles (SEP) as observed in interplanetary space provide fundamental information about the origin of these particles, and the acceleration and propagation processes at the Sun and in interplanetary space. In this paper we review the measurements of ionic charge states of energetic particles in interplanetary space and discuss their implication for our understanding of SEP sources, and acceleration and propagation processes.     

Energization of Plasma Species by Intermittent Kinetic Alfvén Waves

We propose a new phase-mixing sweep model of coronal heating and solar wind acceleration based on dissipative properties of kinetic Alfvén waves (KAWs). The energy reservoir is provided by the intermittent ∼1 Hz MHD Alfvén waves excited at the coronal base by magnetic restructuring. These waves propagate upward along open magnetic field lines, phase-mix, and gradually develop short wavelengths across the magnetic field. Eventually, at 1.5–4 solar radii they are transformed into KAWs. We analyze several basic mechanisms for anisotropic energization of plasma species by KAWs and find them compatible with observations. In particular, UVCS (onboard SOHO) observations of intense cross-field ion energization at 1.5–4 solar radii can be naturally explained by non-adiabatic ion acceleration in the vicinity of demagnetizing KAW phases. The ion cyclotron motion is destroyed there by electric and magnetic fields of KAWs.     

不同温度下DSM11镍基高温合金热腐蚀试验

为了研究DSM11镍基高温合金的抗热腐蚀性能，对该合金在650、750、850℃条件下涂覆5%NaCl+95%Na 2 SO 4 混合盐膜 进行腐蚀试验。利用金相显微镜（OM）、扫描电子显微镜（SEM）、能谱仪（EDS）和X射线衍射仪（XRD）等手段，对合金被腐蚀200 h 后的表面形貌、物相组成、元素和腐蚀层的分布情况以及腐蚀机理进行分析。结果表明：随着试验温度的升高，合金表面腐蚀程度 逐渐加重、腐蚀产物组成逐渐复杂、失重加大、腐蚀产物层厚度增大；合金的腐蚀产物层均可分为3层，最外层和中间层主要为氧 化物，内层由颗粒状氧化物和硫化物组成，O和S的侵入现象表明合金发生了较明显的内氧化与内硫化现象；在3种温度下，合金 表面生成连续稳定的Al 2 O 3 保护层，抑制了热腐蚀反应的进行，对基体存在有效的保护作用，表明合金具有一定的抗热腐蚀性能。