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31.
改进遗传算法的纵列式直升机总体参数优化设计 总被引:1,自引:0,他引:1
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。 相似文献
32.
In this paper we review the possible mechanisms for production of non-thermal electrons which are responsible for the observed
non-thermal radiation in clusters of galaxies. Our primary focus is on non-thermal Bremsstrahlung and inverse Compton scattering,
that produce hard X-ray emission. We first give a brief review of acceleration mechanisms and point out that in most astrophysical
situations, and in particular for the intracluster medium, shocks, turbulence and plasma waves play a crucial role. We also
outline how the effects of the turbulence can be accounted for. Using a generic model for turbulence and acceleration, we
then consider two scenarios for production of non-thermal radiation. The first is motivated by the possibility that hard X-ray
emission is due to non-thermal Bremsstrahlung by nonrelativistic particles and attempts to produce non-thermal tails by accelerating
the electrons from the background plasma with an initial Maxwellian distribution. For acceleration rates smaller than the
Coulomb energy loss rate, the effect of energising the plasma is to primarily heat the plasma with little sign of a distinct
non-thermal tail. Such tails are discernible only for acceleration rates comparable or larger than the Coulomb loss rate.
However, these tails are accompanied by significant heating and they are present for a short time of <106 years, which is also the time that the tail will be thermalised. A longer period of acceleration at such rates will result
in a runaway situation with most particles being accelerated to very high energies. These more exact treatments confirm the
difficulty with this model, first pointed out by Petrosian (Astrophys. J. 557:560, 2001). Such non-thermal tails, even if possible, can only explain the hard X-ray but not the radio emission which needs GeV or
higher energy electrons. For these and for production of hard X-rays by the inverse Compton model, we need the second scenario
where there is injection and subsequent acceleration of relativistic electrons. It is shown that a steady state situation,
for example arising from secondary electrons produced from cosmic ray proton scattering by background protons, will most likely
lead to flatter than required electron spectra or it requires a short escape time of the electrons from the cluster. An episodic
injection of relativistic electrons, presumably from galaxies or AGN, and/or episodic generation of turbulence and shocks
by mergers can result in an electron spectrum consistent with observations but for only a short period of less than one billion
years. 相似文献
33.
基于GRNN网络和遗传算法的旋翼动平衡调整 总被引:1,自引:0,他引:1
针对传统旋翼调整方法没有考虑调整参数与振动信号之间的非线性关系,提出一种结合广义回归神经网络GRNN(General Regression Neural Network)和遗传算法的旋翼调整方法,采用GRNN建立旋翼动平衡调整模型,以桨叶调整参数作为GRNN输入,以旋翼转轴3个方向的加速度测量值和机身3个方向加速度测量值作为网络输出,建立调整参数与直升机振动信号之间的模型.以直升机振动作为目标函数,采用改进的遗传算法对桨叶调整参数进行寻优,获得直升机振动最小时的桨叶的调整量.飞行实验表明,通过1到2次飞行调整,可使3个方向机身振动(旋翼的一阶振动)为最小,完成旋翼的动平衡调整. 相似文献
34.
M. Ishiguro Y. Sarugaku S. Nishihara Y. Nakada S. Nishiura T. Soyano K. Tarusawa T. Mukai S.M. Kwon S. Hasegawa F. Usui M. Ueno 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
Cometary dust trails were first observed by IRAS; they are widely known to be the origins of meteoric showers. A new window has been opened for the study of dust trails, using ground-based observations. We succeeded in obtaining direct images of the 22P/Kopff dust trail with the Kiso 1.05-m Schmidt telescope. Following this initial success, we have continued to perform a dust trail survey at Kiso. As a result of this survey, we have detected dust trails along the orbit of six periodic comets, between February 2002 and March 2004. The optical depth of these dust trails are 10−9 to 10−8, which is consistent with IRAS measurements. In this paper, we describe the observations and data reduction procedures, and report the brief result obtained between February 2002 and March 2004. 相似文献
35.
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。 相似文献
36.
37.
GPS/INS组合系统空中对准方法研究 总被引:3,自引:0,他引:3
针对单天线的GPS与捷联惯性导航组合系统,提出了一种空中对准方案,不同于传统的传递对准方法,仅依靠GPS测量信息进行速度匹配,完成空中初始对准。该方案采用扩展卡尔曼滤波方法解决对准过程中的非线性问题。仿真结果表明该方案的对准精度(1σ)可以达到水平姿态误差0.07,°方位误差0.3°。 相似文献
38.
利用面向对象方法和工作流技术对合作产品定义过程中的分布式工作流管理技术进行研究。建立了合作产品定义过程的动态规划模型和面向对象工作流模型及实现互操作的方法。 相似文献
39.
40.
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。 相似文献