基于6σ设计的复合推力高速直升机总体参数多目标优化

针对复合推力高速直升机总体设计阶段总体参数的选择问题,提出一种提高可靠性和鲁棒性的基于6σ设计的改进多目标遗传算法优化方法。采用叶素理论和数值积分的方法分析计算了复合推力高速直升机气动及飞行性能,并以此为基础建立了约束函数和初步目标函数模型;将6σ设计融入改进的多目标遗传算法中,构造最终目标函数;在给定有效载荷设计要求下,对复合推力高速直升机总体参数进行了多目标优化设计。该方法获得了所需的Pareto解,优化后的复合推力高速直升机飞行性能相对原机有了较大改善,算例结果表明该方法有效可行。     

全数字式操纵负荷系统设计及实现

操纵负荷系统是人在回路仿真系统中的负载模拟装置,它要完成对飞行员十分敏感的驾驶杆力和脚蹬力的仿真,其部件模型的设计满足了操纵负荷系统的通用性。此操纵负荷系统在某型机工程模拟器上的应用测试结果表明,该设计符合直升机飞行模拟器鉴定标准的C级要求。     

改进遗传算法的纵列式直升机总体参数优化设计

研究纵列式双旋翼直升机总体参数的优化设计方法,在分析双旋翼气动干扰对旋翼气动特性影响的基础上,采用改进的遗传算法,以运输效率为目标、以飞行性能和重量效率等参数为约束条件,建立优化设计模型,优化纵列式直升机总体参数。以CH-47D纵列式直升机为优化算例,计算结果表明,本文提出的优化方法是可行的,优化效果良好。     

基于多GPU的大型线性和非线性方程组的求解(英文)

在处理工程问题时,常常需要对线性或非线性方程组进行求解。对于实际应用中经常遇到的大型方程组进行求解则需要相当长的时间。使用图形处理器(GPU)代替传统的CPU,将多块GPU通过操作系统进行协调,并将PBi-CGstab方法和Inexact Newton方法进行适合多GPU并行的改造以此作为多GPU求解器的核心算法,加速求解大型线性和非线性方程组。本文的多GPU求解器在成倍扩展了单GPU求解器允许的计算规模的同时取得了令人满意的加速比。     

一种新的灰色决策模型及其数值仿真(英文)

针对一类权重完全未知且属性值为区间灰数的多指标灰色决策问题,根据灰色理论思想,提出了一种灰色多阶段决策方法。首先给出了一种基于可能度的灰数大小比较方法,然后利用灰色关联分析法对多位专家关于权重的评分结果进行计算得到各指标权重,进而分阶段对指标值以区间灰数的形式进行评分,根据灰色系统新信息优先原理给出了各个阶段评价值的赋权公式。实例验证了该决策方法的可行性。研究结果为求解灰色决策问题提供了一种新思路。     

航电系统集成验证环境中的试验总控系统建设

针对国内军用航空修理行业系统级综合试验现状,根据航电集成验证环境中总控系统的特点和应具有的基本功能,结合视情维修需求及现代软硬件技术状态和成熟试验验证的手段,介绍了航电系统集成验证环境中总控系统的建设思路,给出了总控系统硬件及上位机测试软件的实现方案。该总控系统的应用将提升航电系统的修理验证能力。     

G-16EP通用航空电瓶充放电及寿命研究

为了对G-16EP型电瓶进行维护和保养,根据电瓶厂家规定和适航规范,总结了该型电瓶的充电和容量测试（放电）方法,指出了影响电瓶寿命的主要因素,为该型号电瓶的维护提供了参考。     

Sunspot numbers,interplanetary magnetic field,and cosmic ray intensity at earth: Nexus for the twentieth century

The pivotal role played by the interplanetary magnetic field (B) in modulating galactic cosmic ray (GCR) intensity in the heliosphere is described. We show that the inverse correlation observed by Forbush (1958) between GCRs and sunspot numbers (SSNs) is reflected in high correlation between SSNs and B (cc = 0.94). The SSN data are available since 1700 and the derived B data since 1835. The paleo-cosmic ray data are available for several millennia in the form of ¹⁰Be radionuclide sequestered in polar ice. The data of the ion chambers (ICs) at the Cheltenham–Fredericksburg–Yakutsk (CFY) sites are combined to create a data string for 1937–1988. In turn, these data are used to extend the measurements of the low energy GCR ions (>0.1 GeV) at balloon altitudes at high latitudes in Russia to 1937. These data are then correlated to B and the fit parameters are used to extend the low energy ion data to 1900, creating the instrumental era GCR time series for the twentieth century. The derived GCR time series is compared to ¹⁰Be measured at two sites in Greenland, namely Dye 3 and NGRIP for 1900–2000 to check the internal consistency of datasets for the long-term trend. We find that the annual mean rate (%) for 1965 at NGRIP is an outlier. We replace it with the mean of 1964 and 1965 rates and construct a new re-normalized time series at NGIP, improving the agreement with the derived instrumental era GCR time series for the twentieth century as well. This should encourage its use by heliophysics community for varied applications.     

旋转热源传热特性的理论研究

研究了旋转热源的热传导问题，并将其简化为一维、旋转的周期性脉冲热源传热问题。类似于流体流动，一组新的由旋转角速度ω、热物性参数和几何尺寸组合而成的无量纲拟贝克数Pe1，Pe2．毕奥数Bi被导出。结果表明．它们对传热过程起决定性作用。尤为重要的是，数值仿真对每周转的温度分布给出了微观的“精细”结构和宏观的“粗糙”结构，两的差别取决于上述无量纲数的不同组合，显示了上述几个无量纲准则数的相对关系对传热特性的影响。     

The Crab pulsar seen with AquEYE at Asiago Cima Ekar observatory

We are developing fast photon-counter instruments to study the rapid variability of astrophysical sources by time tagging photon arrival times with unprecedented accuracy, making use of a Rubidium clock and GPS receiver. The first realization of such optical photon-counters, dubbed AquEYE (the Asiago Quantum Eye), was mounted in 2008 at the 182 cm Copernicus Observatory in Asiago. AquEYE observed the Crab pulsar several times and collected data of extraordinary quality that allowed us to perform accurate optical timing of the Crab pulsar and to study the pulse shape stability on a timescale from days to years with an excellent definition. Our results reinforce the evidence for decadal stability of the inclination angle between the spin and magnetic axis of the Crab pulsar. Future realizations of our instrument will make use of the Galileo Global Navigation Satellite System (GNSS) time signal.