导流锥结构参数对燃气弹射筒内压力冲击平滑效果影响研究

针对导流锥结构参数对内弹道流场耦合影响问题，基于动态分层动网格技术，构建了含导弹运动和二次燃烧的内弹道数值模型，并验证了模型可靠性。解耦分析了导流锥半径、高度及冲击高度对内弹道流场特性和载荷的影响。结果表明：导流锥的结构直接决定燃气飞溅现象的产生和流场结构的紊乱程度，导流锥的半径、高度和冲击高度的改变会对燃气反射点的位置、二次燃烧的区域以及剧烈程度产生影响;结构优化后的导流锥，较大程度地缓解了冲击现象，获得了较好的平滑效果，筒底压力较实验装置降低了24.5%。     

制导火箭弹制导控制系统精益设计方法

制导火箭弹在陆军未来战争中正发挥越来越重要的作用，制导控制系统设计是制导火箭弹研制的核心和难题。提出了一种适用于制导火箭弹制导控制系统的精益设计方法，将设计过程分为数据处理环节、自动驾驶仪设计环节、制导律设计环节和六自由度仿真分析环节4个部分，并将标准化和基于模型的思想体现在精益化设计软件中，从而给出了一条可以又快又好地完成系统设计的技术途径。     

1:10人-椅模型上肢的跨-超音速风洞实验

 本文介绍了1:10人椅模型上肢跨-超音速风洞实验的结果。测量了Ma=0.5～2.04和攻角10°～20°范围内上肢的阻力和侧向力。获得了在握扶手和拉中央环两种姿态下手臂的气动力特性。比较了穿衣袖与不穿衣袖两种状态下手臂的气动力数据。实验结果为确定人体上肢对高速气流吹袭的耐久限度和设计防护措施提供了重要的气动力数据。     

基于多维模型的独立型数据集市数据转换策略研究

数据转换是ETL的重要组成部分,同时也是数据仓库和数据集市得到高质量数据的前提和保证。首先分析并研究了基于维度模型的数据转换的内容,提出并深入研究了基于维度模型的独立型数据集市多阶段数据转换策略和管道数据转换策略,为基于多维模型的独立型数据集市的数据转换的实现提供技术支持和理论指导。     

弹射救生过程数值计算及损伤风险评估

针对从弹射程序启动到飞行员着陆之间的各个阶段,建立了能够对横滚、俯冲等复杂弹射条件进行计算的数学模型。结合某型座椅的具体参数与气动力数据,针对具体算例求解了弹射救生过程,与实验结果进行了对比。根据模型的计算结果,以动态响应指数(DRI)对不同弹射初速下的损伤风险做出评估,并指出了在不同速度下气动过载的影响。     

利用喷管引射和旋翼下洗的红外抑制器特性研究

在波瓣引射器一次引射掺混后,提出利用旋翼下洗气流对弯曲混合管排气进行二次强迫混合的红外抑制器结构,并对该红外抑制器进行了有关流动混合特性的实验和数值研究,获得了主流和引射气流、下洗气流相互混合过程中,混合管内部及抑制器出口处的温度场和压力场等相关信息,以及表征引射-混合系统总体性能的引射系数等参数。结果表明:引入下洗气流可以改善出口分布的不均匀性,经过波瓣喷管引射器泵吸周围空气掺混冷却和利用旋翼下洗气流进行二次冷却,可以有效使排气温度降低50%。     

Orientations of LASCO Halo CMEs and their connection to the flux rope structure of interplanetary CMEs

Coronal mass ejections (CMEs) observed near the Sun via LASCO coronographic imaging are the most important solar drivers of geomagnetic storms. ICMEs, their interplanetary, near-Earth counterparts, can be detected in situ, for example, by the Wind and ACE spacecraft. An ICME usually exhibits a complex structure that very often includes a magnetic cloud (MC). They can be commonly modelled as magnetic flux ropes and there is observational evidence to expect that the orientation of a halo CME elongation corresponds to the orientation of the flux rope. In this study, we compare orientations of elongated CME halos and the corresponding MCs, measured by Wind and ACE spacecraft. We characterize the MC structures by using the Grad–Shafranov reconstruction technique and three MC fitting methods to obtain their axis directions. The CME tilt angles and MC fitted axis angles were compared without taking into account handedness of the underlying flux rope field and the polarity of its axial field. We report that for about 64% of CME–MC events, we found a good correspondence between the orientation angles implying that for the majority of interplanetary ejecta their orientations do not change significantly (less than 45 deg rotation) while travelling from the Sun to the near-Earth environment.     

Coronal mass ejection detection using wavelets,curvelets and ridgelets: Applications for space weather monitoring

Coronal mass ejections (CMEs) are large-scale eruptions of plasma and magnetic field that can produce adverse space weather at Earth and other locations in the Heliosphere. Due to the intrinsic multiscale nature of features in coronagraph images, wavelet and multiscale image processing techniques are well suited to enhancing the visibility of CMEs and suppressing noise. However, wavelets are better suited to identifying point-like features, such as noise or background stars, than to enhancing the visibility of the curved form of a typical CME front. Higher order multiscale techniques, such as ridgelets and curvelets, were therefore explored to characterise the morphology (width, curvature) and kinematics (position, velocity, acceleration) of CMEs. Curvelets in particular were found to be well suited to characterising CME properties in a self-consistent manner. Curvelets are thus likely to be of benefit to autonomous monitoring of CME properties for space weather applications.     

弹射座椅弹射筒上连接头挂耳断裂失效分析与研究

本文对弹射座椅弹射筒上连接头挂耳断裂失效现象、安装位置和作用进行了简要介绍;对可能造成上连接头挂耳断裂失效的原材料、尺寸、生产过程、断口、设计及工况强度等主要因素进行了系统排查、分析和验证,最终,找准了零件失效的机理,并准确定位,验证有效,对航空产品提升抗疲劳性能的设计应用起到积极的指导和借鉴意义。     

A Parallel Adaptive 3D MHD Scheme for Modeling Coronal and Solar Wind Plasma Flows

A parallel adaptive mesh refinement (AMR) scheme is described for solving the governing equations of ideal magnetohydrodynamics (MHD) in three space dimensions. This solution algorithm makes use of modern finite-volume numerical methodology to provide a combination of high solution accuracy and computational robustness. Efficient and scalable implementations of the method have been developed for massively parallel computer architectures and high performance achieved. Numerical results are discussed for a simplified model of the initiation and evolution of coronal mass ejections (CMEs) in the inner heliosphere. The results demonstrate the potential of this numerical tool for enhancing our understanding of coronal and solar wind plasma processes. This revised version was published online in June 2006 with corrections to the Cover Date.