机载计算机ATE计量校准软件的研究与设计

全面有效地计量校准军用ATE,对保证其正确性有效性非常重要.设计开发ATE计量校准程序,可以实现ATE自动化整体原位校准,提高计量保障效率和测试质量.介绍了机栽计算机ATE计量校准软件的系统结构,重点讨论了计量校准程序结构和面向信号的程序开发方法,最后描述了计量校准程序流程和实现方法.     

基于可压缩格子Boltzmann方法的高可扩展并行算法研究

Lattice Boltzmann Methods(LBM)是近年来发展的求解流体问题的计算新方法,该方法具有编程相对简单,并行计算效率高的特点,但是现有的D2Q9 LBM模型只能计算速度在0.3马赫下的不可压缩流体,提出的新的LBM模型可以处理速度0.7马赫以下的流体问题,并且具有较好的数值稳定性,对计算程序并行性能深入研究的基础上,提出了基于cache的性能优化,经过程序性能测试证明该方法具有较好并行计算效率,并具有很好的可扩展性.     

飞行间隔安全评估研究

 首先概述了飞行间隔安全评估研究中常用的概念,然后从REICH模型、交叉航路模型、概率论模型、随机分析模型、EVENT模型和RASRAM模型6种常用碰撞风险模型的角度,分析了各个模型的优缺点和各自的适用范围,分析结果表明飞行间隔安全评估中的关键问题为：模型的限制、管制意图和安全评价,并在此基础上分析了飞行间隔安全评估未来的研究方向。     

剪切翼尖对机翼气动效能影响研究

尖切翼尖作为一种重要的翼尖装置,由于实现简单,能有效得减小机翼得诱导阻力且对飞机的其它性能影响小,而受到广泛的应用.基于数值模拟结果对尖切翼尖的前缘后掠角及根梢比对机翼气动性能的影响进行了对比研究.给出了前缘后掠角和根梢比对气动性能的影响规律,并通过分析涡位置和强度的变化,得出涡位置及强度和气动性能的关系.     

一种同轨区域集中的北斗卫星自主导航算法

基于北斗三号卫星配置规划,提出了一种同轨区域集中的北斗卫星自主导航算法。利用Ka星间链路指向切换灵活特性与激光链路高速通信特性,并克服激光终端异轨面通信困难,指向切换不便等缺陷,算法设计将轨道面内各卫星采集的Ka双向测距信息利用激光星间链路传入轨道面主卫星中,从而将测距信息集中处理并完成轨道面内各卫星的轨道信息更新。并且,本文还搭建了星内模拟仿真环境,对算法精度及性能进行验证。仿真结果表明,同轨道区域集中自主导航算法可在星内仿真环境中稳定运行,且其导航精度远优于分布式自主导航精度。     

合成双射流逆向吹吸控制对翼型流动特性影响

为探究合成双射流(Dual?Synthetic?Jets,DSJ)技术对飞行器航向姿态的控制能力,采用数值模拟的方法,研究了反向DSJ对小攻角、大攻角下翼型绕流流场的控制机理及气动控制特性,并通过飞行试验验证了其航向姿态控制能力.结果表明:小攻角下,反向DSJ会使阻力增大,升力略有减小,俯仰力矩基本不变;大攻角下,反向DSJ会使升力、阻力及低头力矩增大.小攻角下施加控制后,激励器出口前由于射流的阻挡作用形成高压区,伴随着流向逆压梯度的增加,分别在两个出口后形成准定常低压回流区,致使前后压差阻力增大,但压力包络面积基本不变,故升力变化不大;大攻角下施加控制后,除了会在射流出口前、后分别形成高压区、低压区外,还会使背风面流动提前分离,扩大分离区域面积,同时也会减小分离区内的压力值,扩大压力包络,增大阻力的同时,也会提升升力.飞行试验结果表明,反向DSJ具有对飞行器巡航时航向姿态的控制能力,可实现的最大偏航角速度为9.01°/s.     

翱翔系列立方星的发展和展望

针对西北工业大学“翱翔”系列立方星在低成本、短周期、快响应的立方星技术方面的突破，介绍了应用于大气层外偏振导航技术试验的世界首颗12U立方星“翱翔之星”，世界首次组网开展低热层大气参数测量的QB50计划“翱翔一号”立方星等，总结了“翱翔”系列立方星的标准化结构设计、姿态控制系统、电源系统、星载计算机、通信与测控、部署器等核心系统的发展现状，介绍了自主研制的飞轮、磁力矩器、偏振敏感器载荷。并基于在轨组装，编队飞行，一箭多星等技术对“翱翔”系列立方星的应用进行了展望，对探索柔性、高精度、长寿命的立方星将有重要的意义。     

基于优化STD法的大飞机垂尾装配界面精加工过程模态参数识别

为减小大飞机垂尾装配界面精加工过程中产生的加工振动对其精加工质量的影响，需掌握装配界面加工过程的动力学特性，而动力学特性与其模态参数密切相关。因此，为获得装配界面各阶模态参数，针对其动态精加工过程，提出了一种优化STD环境激励下结构模态参数识别方法。该方法首先由装配界面的实测加工振动数据构造Toeplitz矩阵，并将其作为STD法的输入，进而求出装配界面各阶次模态参数，并构成模态参数下三角矩阵。然后利用模态置信因子及模态保证准则选出阶次相对稳定的模态参数作为装配界面的真实模态参数。最后，通过切削实验和锤击测试验证优化STD法的正确性和有效性。将锤击实验模态结果作为装配界面的模态参数测量参考值，以一阶模态频率识别结果为例，该方法相比于传统STD法和SSI法，识别精度分别提高了12.71%和3.82%；同理其余各阶模态参数识别精度均有不同程度的提高。通过优化STD法可准确高效地获得装配界面的模态参数，为其精加工工艺参数的合理选择提供了理论依据和技术支持。     

QB50 Project and the Development of Cube Sat Technology in China

The Cube Sat refers to the low-cost nano satellite produced by international standards. The QB50 project is "an International Network of 50 double Cube Sats for multi-point, in-situ, long-duration measurements in the lower thermosphere and re-entry research". There are 23 countries and region participated in the QB50 Project. 38 Cube Sats were developed and launched. Among them, four Cube Sats developed by Chinese universities were sent to orbit(Three were deployed from the International Space Station, and one was launched by the Polar Satellite Launch Vehicle, PLSV). They are Aoxiang-1(Northwestern Polytechnical University, the Asia coordinator), Lilac Sat-1(Harbin Institute of Technology), NJUST-2(Nanjing University of Science and Technology) and NUDTsat(National University of Defense Technology). Through the development of the QB50 Project, Chinese researchers and students got in touch with the concept of Cube Sat and gained experience of international scientific cooperation. A lot of students took part in the assembly, integration, and test of spacecraft, which is helpful to the training of space talents. Now, many universities and institutes have the capabilities to develop Cube Sats and the subsystems independently.     

Can an impulsive variation of the solar wind plasma pressure trigger a plasma bubble? A case study based on CSES,Swarm and THEMIS data

During the August 25, 2018 geomagnetic storm, the new borne CSES-01 satellite and the Swarm A satellite detected a really large equatorial plasma bubble (EPB) in the post-midnight sector over western Africa. We investigated the features of this deep ionospheric plasma depletion using data from the Langmuir probes on-board CSES-01 and Swarm A satellites, and data from the high-precision magnetometer and the electric field detector instruments on-board CSES-01. Using also plasma and magnetic field data from THEMIS-E satellite we found that, during the passage of the magnetic cloud that drove the geomagnetic storm, an impulsive variation lasting about ten minutes characterized the solar wind (SW) pressure. The analysis of the delay time, between the occurrence of such impulsive variation and the detection of the plasma bubble, suggests a possible link between the SW pressure impulsive variation as identified by THEMIS-E and the generation of the EPB as detected by CSES-01 and Swarm A. We put forward the hypothesis that the SW pressure impulsive variation might have triggered an eastward prompt penetrating electric field that propagated from high to equatorial latitudes, overlapping in the nightside region to the zonal westward electric field, causing either a reduction or an inversion, at the base of the EPB triggering.