N5B飞机机身钢构架焊接架数字化设计与制造技术

详细阐述了在N5B飞机机身钢构架焊接架的设计与制造中运用数字化技术的先进性。     

高超声速飞行器后体喷管三维构型设计

为研究高超声速飞行器后体喷管三维构型的设计,以NASA半壁喷管试验为参考,进行了二维及三维内外流相互作用的数值模拟计算,分析了后体喷管三维流场的特点.从高超声速飞行器机身推进一体化的角度,构建了后体喷管三维构型,进行了不同构型设计对后体喷管性能影响的参数研究.结果表明:后体喷管的三维效应不可忽视,后体喷管侧壁的存在及下壁面长度对性能影响较大.      

小型化1553B通信协议芯片Mini—ACE的开发和应用

为满足MBI模块小型化、轻型化、低功耗、高可靠性和灵活性的要求,设计一块采用TI公司小型DSP处理器SM320F2812作为处理器、DDC公司小型化BU61865芯片作为协议芯片,采用FP—GA实现主要逻辑的双路、双余度、双通道MBI。该MBI能极大地减小总线负载,提高总线传输效率.Mini—ACE使得MBI具有总线控制器、远程终端、总线监控器、组合远程终端和选择消息监控等功能。通过在系统单位的综合与联试,该MBI模块能够满足系统的快速、灵活等要求．     

Modelling of galactic Carbon in an asymmetrical heliosphere: Effects of asymmetrical modulation conditions

Observations of galactic cosmic rays (GCRs) from the two Voyager spacecraft inside the heliosheath indicate significant differences between them, suggesting that in addition to a possible global asymmetry in the north–south dimensions (meridional plane) of the heliosphere, it is also possible that different modulation (turbulence) conditions could exist between the two hemispheres of the heliosphere. We focus on illustrating the effects on GCR Carbon of asymmetrical modulation conditions combined with a heliosheath thickness that has a significant dependence on heliolatitude. To reflect different modulation conditions between the two heliospheric hemispheres in our numerical model, the enhancement of both polar and radial perpendicular diffusion off the ecliptic plane is assumed to differ from heliographic pole to pole. The computed radial GCR intensities at polar angles of 55° (approximating the Voyager 1 direction) and 125° (approximating the Voyager 2 direction) are compared at different energies and for both particle drift cycles. This is done in the context of illustrating how different values of the enhancement of both polar and radial perpendicular diffusion between the two hemispheres contribute to causing differences in radial intensities during solar minimum and moderate maximum conditions. We find that in the A > 0 cycle these differences between 55° and 125° change both quantitatively and qualitatively for the assumed asymmetrical modulation condition as reflected by polar diffusion, while in the A < 0 cycle, minute quantitative differences are obtained. However, when both polar and radial perpendicular diffusion have significant latitude dependences, major differences in radial intensities between the two polar angles are obtained in both polarity cycles. Furthermore, significant differences in radial intensity gradients obtained in the heliosheath at lower energies may suggest that the solar wind turbulence at and beyond the solar wind termination shock must have a larger latitudinal dependence.     

相位自动跟踪检测系统

介绍一种适用于自动化的相位跟踪检测系统。该系统采用新的相位测量方法——平均相位角法,消除了过零触发电路中固有的直流电平带来的相位偏移引起的相位测量误差。同时,设计了新颖的用于自动测量的相对计数时间/频率转换电路,在激光干涉比长仪1m行程内实时检测相位变化,保证了激光干涉比长仪的测量精度,提高了自动化程度。     

基于人工鱼群算法的单机场地面等待优化策略

目前大型机场拥塞问题日益严重.推迟飞机起飞时间,将成本较高的空中等待转化成地面等待,是进行空中交通流量管理的一个有效方法.本文研究基于人工鱼群算法的单机场地面等待优化策略并进行仿真,有效地减少了总的地面等待延误损失,说明该方法是可行的;通过与其他几种智能算法的比较,验证了该算法执行效率高、实用性强.     

建筑物风环境三维定常数值仿真

针对建筑物的风环境问题，采用计算流体动力学CFD软件对两幢建筑物进行了数值模拟，得出了建筑物的风场分布，以及风载的分布规律，结果表明，气流在来流方向第一幢建筑物的顶部、两侧的前沿产生分离，建筑物之间产生强烈的漩涡，顶部的局部负压最大。     

阶梯波合成整流器及其调制策略

提出了基于阶梯波合成结构的整流器,具有开关频率低、谐波含量小、滤波器体积小、输入功率因数和输出电压可控等优点,非常适合大功率应用场合.详细介绍了其工作原理.分析了输出电压调节方法,并提出采用具有特殊采样时序的错时采样空间矢量调制方法对其进行PWM调节,既保留了阶梯波合成技术的消谐波能力又使得交流侧合成电压的相位和幅值可调,以便于实现输入单位功率因数和输出直流电压的调节,最后通过实验验证了该阶梯波合成整流器的可行性.     

无人机舵回路及其新型控制策略设计和应用

以无人直升机飞行控制系统研制实际需要为背景,运用高集成AVR单片机设计了数字式舵回路控制器,根据嵌入式计算机系统实现舵回路控制律要求,设计并实现了舵回路数字式控制律.采用变参数调节控制律可使舵回路控制性能达到理想状态,有效避免了系统超调和积分饱和.舵回路控制参数的在线调整,实现了不同被控对象/不同状态的有效控制,拓展了数字式舵回路的适用场合.在综合汲取伺服电机调制模式基础上,提出了复合PWM模式和"极性比"概念,实现了数字式舵回路低功耗之目的.文中给出了部分试验结果和应用实例.结果表明,所设计的低功耗数字式舵回路是成功的,该舵回路不但功耗低,体积小,而且抗干扰能力强.     

X-Ray spectroscopic investigation of the coronal structure of capella

The binary system Capella (G6 III + F9 III) has been observed on 1979 March 15 and on 1980 March 15–17 with the Objective Grating Spectrometer (OGS) onboard theEinstein Observatory. The spectrum measured with the 1000 l/mm grating covers the range 5–30 Å with a resolution < 1 Å. The spectra show evidence for a bimodal temperature distribution of emission measure in an optically thin plasma with one component 5 million degrees and the other one 10 million degrees. Spectral features can be identified with line emissions from O VIII, Fe XVII, Fe XVIII, Fe XXIV, and Ne X ions. Good spectral fits have been obtained assuming standard cosmic abundances. The data are interpreted in terms of emission from hot static coronal loops rather similar to the magnetic arch structures found on the Sun. It is shown that the conditions required by this model exist on Capella. Mean values of loop parameters are derived for both temperature components.