磁力矩器用聚合物材料的原子氧效应试验研究

文章对磁力矩器用4种聚合物材料进行原子氧和真空效应评价试验,利用新型的原子氧环境模拟设备及其他分析手段对试样的质量损失率(SAML)和表面形貌的变化进行了研究。试验结果表明,真空环境会导致材料产生质量损失,4种材料的真空质损最大相差24倍;原子氧作用导致聚合物材料的颜色发生变化,且造成材料的质量损失,4种材料的质量损失率最大相差25倍;原子氧与有机硅物质反应能够形成保护层,可以抑制原子氧对材料内部的进一步侵蚀。     

移动质心飞行器的参数辨识和补偿控制

受质量块大小和位移的限制,移动质心不能像空气舵那样产生很大的力矩.因此飞行器的再入攻角对静稳定度很敏感,尤其在小静稳定度下,静稳定度稍有改变,配平攻角将发生很大变化.飞行器再入过程中的烧蚀、侵蚀以及边界层转捩所造成的小不对称量所产生的不对称力矩与质心移动后产生的控制力矩相比,不是小量.以所建立的移动质心控制飞行器的数学模型为基础,辨识飞行器静稳定度和小不对称量,对小不对称量造成的气动力矩用前馈一反馈复合控制加以补偿.仿真分析表明,移动质心控制对高速再入的飞行器具有良好的末修能力,能有效提高再入段的控制精度.     

螺旋桨-自由涡轮涡桨发动机稳态/过渡态数值模拟

为实现对涡桨推进系统整体推进性能的数学模型模拟,以螺旋桨/桨扇作为受飞行外流条件影响的推进系统内流部件之一,引入其特性图,用跟随流量方法解决螺旋桨-自由涡轮转子与涡桨发动机燃气发生器的流量平衡、功率平衡,发展了螺旋桨-自由涡轮涡桨发动机内流特性部件法数学模型,实现了对该类涡桨系统稳态/过渡态的数值模拟。对某8MW三轴桨扇发动机的台架转速特性和飞行任务剖面特性的数值模拟结果表明:该数学模型可以较为准确模拟出包含桨叶变动桨距角、攻角等在内的外流螺旋桨/桨扇部件工作点详细参数,和高度、速度、涡轮前温度同时变化的多条件、多变量涡桨发动机的稳态/过渡态推力、推力耗油率等特性.      

低温燃气弹射内弹道影响因素的数值研究

针对某低温燃气式弹射装置,建立简化二次燃烧物理模型,采用重整化群k-ε湍流模型模拟流场流动、以有限速率/涡耗散燃烧模型模拟气相燃烧、以域动分层法动网格更新技术模拟导弹运动,数值分析得到了发射筒内载荷与内弹道特性.结果表明:在满足内弹道设计要求的条件下,燃气发生器喷管入口总温包络区间为0.538~1.231,且随着总温的增加,二次反应时间和导弹出筒时间减小,导弹出筒速度增加;发射筒内氧气质量分数包络区间为0.07~0.30,且随着氧气质量分数的增加,二次反应发生时间和导弹出筒时间提前,导弹出筒速度增加.研究结果可为低温燃气式弹射内弹道分析和结构设计提供理论基础.      

民用飞机虚拟维修可达性技术研究

结合民用飞机维修性设计的要求和特点,将虚拟现实技术引入到飞机维修性设计、分析与验证工作中,阐述了虚拟维修仿真的流程。通过可视性分析、实体可达分析、操作空间分析,给出了虚拟维修的可达性验证方法,实现设计中的维修性设计评价,从中找出影响维修性设计的因素进而及时改进,以提高整机维修性。     

航天器虚拟热试验平台的软件架构及其应用

针对我国目前航天领域型号试验任务重、成本高的特点,文章提出搭建航天器虚拟热试验平台以缩短型号研制周期、减少研发成本。虚拟热试验平台结构拟由5个单独模块组成:试验系统描述及边界条件输入模块,虚拟试验运算模块,模型修正模块,结果报表及经济性分析模块和虚拟试验数据库。另外提出了虚拟热试验平台在航天器真空热试验中的应用。     

Interface Familiarity Restores Active Advantage in a Virtual Exploration and Reconstruction Task in Children

Abstract

Active exploration is reportedly better than passive observation of spatial displacements in real environments, for the acquisition of relational spatial information, especially by children. However, a previous study using a virtual environment (VE) showed that children in a passive observation condition performed better than actives when asked to reconstruct in reality the environment explored virtually. Active children were unpractised in using the input device, which may have detracted from any active advantage, since input device operation may be regarded as a concurrent task, increasing cognitive load and spatial working memory demands. To examine this possibility, 7–8-year-old children in the present study were given 5 minutes of training with the joystick input device. When compared with passive participants for spatial learning, active participants gave a better performance than passives, placing objects significantly more accurately. The importance of interface training when using VEs for assessment and training was discussed.     

CONTROL OF TWO DIMENSIONAL JETS USING MINIATURE ZERO MASS FLUX JETS

Zero mass flux jets, synthesized by acoustic actuators, have been used for the purpose of jet mixing enhancement and jet vectoring. Zero mass flux jets composed of entirely entrained fluid allow momentum transfer into the embedding flow. In the present experiments, miniature-scale high aspect ratio actuator jets are placed along the long sides and near the exit plane of a primary two-dimensional jet. In different modes, the primary jet can be vectored either towards or away from the actuator jets and the jet mixing is enhanced. The disturbance of the excitation frequency is developed while the unstable frequency of the primary jet is completely suppressed.     

ATM局域网仿真技术

简要介绍了 Ａ Ｔ Ｍ 局域网仿真的主要原理，以 Ｉ Ｂ Ｍ ８２６０ Ａ Ｔ Ｍ 交换机为例，具体分析了 Ａ Ｔ Ｍ 局域网仿真的实现细节。     

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.