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761.
基于径向基函数响应面的机翼有限元模型修正 总被引:2,自引:1,他引:1
用ANSYS三维实体单元SOLID45建立机翼基准有限元模型并计算其自由振动的前6阶模态频率.用均匀设计方法将结构参数分组并分别计算各组结构参数对应的模态频率,建立高斯径向基函数响应面模型.用最小二乘法则拟合系数并检验响应面拟合精度,对基准模型的结构参数施加摄动量建立待修正有限元模型.用响应面模型和基准模型计算所得模态频率的相对误差建立适应度函数的表达式,将混沌搜索机制引入粒子群算法对结构参数的摄动量进行寻优计算,搜索所得优化解代入即得修正后模型,将修正后模型与基准模型在测试频段内段外的模态频率近似度进行比较,证实了修正后模型的有效性. 相似文献
762.
物理规划方法及其在飞机方案设计中的应用 总被引:3,自引:0,他引:3
物理规划方法是一种高效的设计优化方法,它与设计者的工程经验紧密联系,能以较低的计算代价获得真实反映设计者偏好的折衷解,对解决多目标优化设计问题具有重要意义。将物理规划设计方法与稳定、高效的粒子群优化算法相结合,有效地求解多目标优化问题中的折衷非劣解。通过求解数值算例和民用飞机方案设计问题,验证了该方法的有效性。 相似文献
763.
目标威胁评估是空战对抗过程中的关键环节。由于影响空战目标威胁评估的因素复杂多样,且指标之间存在相关性,导致传统的评估算法无法得到准确客观的评估结果。由此,提出了一种基于主成分分析法和改进粒子群算法优化的极限学习机(PCA-MPSO-ELM)的目标威胁评估算法。首先,综合分析了影响目标威胁程度的指标,利用主成分分析法对原始评估指标进行线性变化处理得到综合变量,消除了评估指标之间的相关性,实现了对评估数据的降维;在此基础上,构建ELM神经网络并利用改进的粒子群算法优化极限学习机的输入权值和阈值,提高了目标威胁评估模型的精度。最后,在空战训练测量仪中选取空战对抗数据,利用威胁指数法构造了目标威胁评估样本数据,通过仿真实验分析了PCA-MPSO-ELM算法的精度和实时性,结果表明所提算法可以快速准确地进行空战目标威胁评估。 相似文献
764.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2023,71(3):1840-1854
We present an analysis of the time-intensity profiles of 25 solar energetic proton events at 18.2 MeV, modelled by fitting an analytical function form (a modified Weibull function) to the observed intensities. Additionally relying on previous work that characterized the magnetic connectivity between the event-related solar flare and the observer in these events with three angular parameters, we investigate the fit function parameters, the connectivity parameters, and the iron-to-carbon ratio of the events for dependencies and correlations. We find that the fit parameter controlling the basic shape of the profile (parameter a) is not clearly dependent on the connectivity parameters or the Fe/C ratio, suggesting that the profile shapes of neither well and weakly connected nor generally “impulsive” and “gradual” events differ systematically during the early stages of the event at 1 AU. In contrast, the time scaling of the fit function (parameter b) is at least moderately correlated with both the magnetic connectivity parameters and the Fe/C ratio, in that well-connected and iron-rich events are typically shorter in relative duration than weakly connected and nominal-abundance events; intensity rise times display a similar correlation with the connectivity parameters. We interpret the former result as following from the combined effect of various transport processes acting on the particles in interplanetary space, while the latter is essentially consistent with established knowledge regarding the observed dependence of the time-intensity profile shapes of solar energetic particle events on their magnetic connectivity and heavy ion abundances. The desirability of modelling the particle transport effects in detail and extending the analysis to cover higher energies is indicated. 相似文献
765.
766.
767.
《中国航空学报》2020,33(5):1532-1540
Location layout of aircraft assembly is an important factor affecting product quality. Most of the existing re-searches use the combination of finite element analysis and intelligent algorithm to optimize the location layout, which are limited by numerical simulation accuracy and the selection and improvement of intelligent algorithms. At present, the analysis and decision-making technology based on field data is gradually applied in aircraft manufacturing. Based on the perception data of intelligent assembly unit of aircraft parts, a regression model of multi-input and multi-output support vector machine with Gauss kernel function as radial basis function is established, and the hyperparameters of the model are optimized by hybrid particle swarm optimization genetic algorithm (PSO-GA). GA-MSVR, PSO-MSVR and PSOGA-MSVR model are constructed respectively, and their results show that PSOGA-MSVR model has the best performance. Finally, the design of the aircraft wing location layout is taken as an example to verify the effectiveness of the method. 相似文献
768.
Xiaocan Li Brahmananda Dasgupta Gang Li 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
We investigate the acceleration of charged particles in a time-dependent chaotic magnetic field in this work. In earlier works, it has been demonstrated that in an asymmetric wire-loop current systems (WLCSs), the magnetic field is of chaotic in nature. Furthermore, observations also showed that there exist time-varying current loops and current filaments in solar corona. It is therefore natural to conceive that the magnetic field on the solar surface is chaotic and time-dependent. Here, we develop a numerical model to study the acceleration process of charged particles in a time-varying chaotic magnetic field that is generated by an ensemble of 8 WLCSs. We found that the motion of energetic particles in the system is of diffusive in nature and a power law spectrum can quickly develop. The mechanism examined here may serve as an efficient pre-acceleration mechanism that generates the so-called seed particles for diffusive shock acceleration at a coronal mass ejection (CME) driven shock in large solar energetic particle (SEP) events. 相似文献
769.
770.
以双基地雷达"四抗"能力分析为基础,提出了双/多基地雷达布站优化的原则并对这些原则进行了量化,建立了双/多基地雷达布站优化的数学模型.随后,对量子粒子群算法进行了改进,提出了自适应量子粒子群算法,并将其用于双/多基地雷达布站优化数学模型的求解,解决了双/多基地雷达雷达站的部署问题.最后,通过MATLAB对优化后的雷达站... 相似文献