T型尾翼颤振模型光学测量实验与弯扭特性解算

在FL-26跨声速风洞半模试验段进行了某高速飞机T型尾翼颤振模型的光学测量实验,并依据测量结果解算了尾翼颤振模型的弯扭特性。颤振模型表面用白色圆点进行标记,用于记录模型表面的位移变化,两台固定在风洞试验段上壁板观察孔旁肋板上的400万像素工业相机用来采集图像,采集到的图像通过自主开发的图像解算软件进行图像的识别与求解,计算出尾翼颤振模型表面标记点的三维坐标。模型表面标记点的三维坐标通过坐标变化转换到风洞气流坐标系中,利用不同时刻模型表面坐标的变化计算模型剖面扭角和弹性轴位移的分布。T型尾翼右平尾图像采集实验与弯扭特性计算结果表明,非接触光学测量技术可以用于高速颤振试验的定量分析中。     

Introduction

Space Science Reviews -     

Solar Wind Electron Proton Alpha Monitor (SWEPAM) for the Advanced Composition Explorer

The Solar Wind Electron Proton Alpha Monitor (SWEPAM) experiment provides the bulk solar wind observations for the Advanced Composition Explorer (ACE). These observations provide the context for elemental and isotopic composition measurements made on ACE as well as allowing the direct examination of numerous solar wind phenomena such as coronal mass ejections, interplanetary shocks, and solar wind fine structure, with advanced, 3-D plasma instrumentation. They also provide an ideal data set for both heliospheric and magnetospheric multi-spacecraft studies where they can be used in conjunction with other, simultaneous observations from spacecraft such as Ulysses. The SWEPAM observations are made simultaneously with independent electron and ion instruments. In order to save costs for the ACE project, we recycled the flight spares from the joint NASA/ESA Ulysses mission. Both instruments have undergone selective refurbishment as well as modernization and modifications required to meet the ACE mission and spacecraft accommodation requirements. Both incorporate electrostatic analyzers whose fan-shaped fields of view sweep out all pertinent look directions as the spacecraft spins. Enhancements in the SWEPAM instruments from their original forms as Ulysses spare instruments include (1) a factor of 16 increase in the accumulation interval (and hence sensitivity) for high energy, halo electrons; (2) halving of the effective ion-detecting CEM spacing from ∼5° on Ulysses to ∼2.5° for ACE; and (3) the inclusion of a 20° conical swath of enhanced sensitivity coverage in order to measure suprathermal ions outside of the solar wind beam. New control electronics and programming provide for 64-s resolution of the full electron and ion distribution functions and cull out a subset of these observations for continuous real-time telemetry for space weather purposes. This revised version was published online in June 2006 with corrections to the Cover Date.     

Rocket berthing to an asteroid: Design problems

The results of research in a process of a probe rocket berthing to an asteroid are presented. Control laws were obtained as solutions of three problems, namely berthing considering transient processes in a rocket engine, fastest berthing with regard to fuel consumption and berthing in a scheduled time considering fuel consumption. A program trajectory obtained at solving of the first problem is suitable for mathematical modeling of berthing with the feedback control law and stabilization of angular motion. The solutions of the problems are reduced to simple formulas for controlling parameters calculation in the corresponding structures of control laws. The results can be applied in designing promising space vehicles intended for berthing to other space objects.     

电磁兼容性标准的剪裁及应用

依据有关的电磁兼容性标准,并结合国内外的情况,着重对电磁兼容性标准剪裁的必要性、方式、方法、时机和分工问题进行了论述,同时提出在项目剪裁中应注意的问题。     

基于细观颗粒夹杂模型的复合固体推进剂松弛模量预测

为更准确地预测不同固体颗粒体积分数的复合固体推进剂的松弛模量,采用了分子动力学方法对不同体积分数的复合固体推进剂细观模型进行建模.根据有限元理论及细观力学均匀化方法,计算在定应变工况下复合固体推进剂细观模型的平均应力随时间的变化,从而有效地预测复合固体推进剂的松弛模量.该方法有效地体现了随填充颗粒体积分数的增大,复合固体推进剂瞬时模量逐渐增大的变化规律及颗粒随机分布对复合固体推进剂瞬时模量的影响.将其应用到复合固体推进剂的设计过程中,可有效降低设计成本,缩短设计周期.      

基于FPGA的半球谐振陀螺频率跟踪技术

半球谐振陀螺谐振频率的跟踪精度与稳定性很大程度上决定了陀螺的性能。通过分析半球谐振陀螺的频率特性以及锁相环基本原理,设计了基于锁相环的半球谐振陀螺频率跟踪方案,并用FPGA进行全数字化实现。半球谐振陀螺采用真空封装,内部温度难以测量,然而其谐振频率与温度具有很好的线性相关性,因此可采用谐振频率对陀螺温度进行测量。传统的频率跟踪方案一般采用模拟锁相环实现,其缺点是频率值隐含于输出的正弦波中,无法供后继测量模块使用,本文所设计的FPGA全数字方案可弥补这一缺陷。根据陀螺谐振频率与温度之间的关系,给出了利用跟踪频率测温的分辨率公式并进行了相关实验。实验结果显示,谐振频率为4440Hz时频率跟踪稳态相对误差可达10-7量级,利用跟踪频率测温的分辨率可达0.0042℃。     

Elemental Abundances in Coronal Structures

A great deal of evidence for elemental abundance variations among different structures in the solar corona has accumulated over the years. Many of the observations show changes in the relative abundances of high- and low-First Ionization Potential elements, but relatively few show the absolute elemental abundances. Recent observations from the SOHO satellite give absolute abundances in coronal streamers. Along the streamer edges, and at low heights in the streamer, they show roughly photospheric abundances for the low-FIP elements, and a factor of 3 depletion of high-FIP elements. In the streamer core at 1.5 R·, both high- and low-FIP elements are depleted by an additional factor of 3, which appears to result from gravitational settling. This revised version was published online in June 2006 with corrections to the Cover Date.     

某民用飞机机身典型壁板压损分析

通过RADIOSS显示有限元计算,对典型壁板结构的承载能力进行了计算分析,并与试验结果进行对比,验证了RADIOSS显式有限元计算分析的准确性。在此基础上,针对某民用飞机的机身壁板5种不同的典型壁板结构,分别在长度为200 mm和530 mm的情况下,采用有限元分析方法计算了长桁及壁板结构的压损和失稳情况,最终得出5种构型下的压损及失稳结果,为机身结构共性结构选型提供了数据支持。     

粒子分离器砂尘分离效率试验参数影响分析

砂尘试验是评估和验证粒子分离器砂尘分离能力的核心方法,砂尘分离效率试验结果除受试验器测试精度影响,还与 砂尘投放方式直接相关。为了摸清某粒子分离器砂尘分离效率的试验影响因素,结合流动机理分析、CFD仿真和试验方法,分别 针对粒子分离器进口粒子分布均匀性、砂尘浓度和喷砂速度3种因素对砂尘分离效率的影响进行了分析。结果表明：粒子分离器 进口砂尘分布均匀性是影响砂尘试验结果的主要因素,在给定浓度分布模型下,进口砂尘非均匀分布比非均匀分布砂尘分离效率 降低接近7%;进口砂尘浓度在2000 mg/m3范围内变化不会对分离效率试验结果产生显著影响;喷砂速度增大,大粒径粒子受壁面 反弹影响,使粒子分离器总分离效率呈下降低趋势。