期刊文献+

混合粒子群算法ADPSO对月球物理参数反演的改进 被引量:4

Lunar Geophysical Parameter Inversion with Admixed Particle Swarm Optimization ADPSO
下载PDF
导出
摘要 常规粒子群算法PSO对低敏感参数较难进行最优估计,本文提出联合自适应惯性权重和变异的混合粒子群算法ADPSO.结果表明:最佳拟合效果不随粒子数和变异概率的增大而加强.就四参数估计而言,粒子数取400个,变异概率小于0.03,可实现最优拟合.采用最佳粒子数和较小的变异概率,利用新近月球重力场模型GL0990d和LRO激光测高数据,对月球南半球部分高地的物理参数进行最优估计.发现研究区域的模型导纳谱很好地拟合了观测值,模型重力异常与观测重力异常的残差较小,符合参数估计的要求,验证了算法的有效性.ADPSO适合于月球物理参数估计,为大规模的反演运算提供了参考. Ordinary particle swarm optimization PSO fails frequently in estimation of low sensitivity selenophysics parameters.With an adaptive inertia weight and a mutation factor,an admixed particle swarm optimization ADPSO is proposed.It is found that misfit is not reduced as increasing number of particles and probability of mutation.For four-parameter inversion,the best-fitting parameters can be estimated as considering about 400 particles and a low probability(0.03) of mutation.With employment of gravity filed model GL0990 d and altimeter data from LRO,we apply the method into selenophysical parameter inversion on southern highland of the moon.It shows a best-fit between modeled admittance spectral and observed values.Small residual of gravity anomaly verifies success of parameter inversion and validity of the method.The approach can be used in selenophysics research and could provide a reference for large-scale estimation of parameters.
作者 钟振
出处 《计算物理》 CSCD 北大核心 2017年第6期740-746,共7页 Chinese Journal of Computational Physics
基金 国家自然科学基金(41404021) 贵州省科学技术基金(黔科合J字[2014]2128) 贵州师范大学博士科研项目资助
关键词 月球物理 参数估计 混合粒子群 导纳谱 selenophysics parameter estimation admixed particle swarm admittance spectral
  • 相关文献

参考文献4

二级参考文献62

  • 1鄢建国,平劲松,李斐,王威.应用LP165P模型分析月球重力场特征及其对绕月卫星轨道的影响[J].地球物理学报,2006,49(2):408-414. 被引量:28
  • 2李斐,鄢建国,平劲松.月球探测及月球重力场的确定[J].地球物理学进展,2006,21(1):31-37. 被引量:28
  • 3刘华蓥,林玉娥,张君施.基于混沌搜索解决早熟收敛的混合粒子群算法[J].计算机工程与应用,2006,42(13):77-79. 被引量:32
  • 4Lewis B T R, Dorman L M. Experimental Isostasy 2: An isostatic model for the USA derived from gravity and topographic data. J. Geophys. Res. , 1970,75 (17) : 3367-3386.
  • 5Willemann R J, Turcotte D L. Support of topographic and other loads on the moon and on the terrestrial planets. Proc. Lunar Planet Sci. ,1981, B12:837-851.
  • 6Prasons B, Slater J G. An analysis of the variation of the ocean floor bathymetry and heat flow with age. J. Geophys. Res. , 1977,82(5) :803-827.
  • 7Crosby A, McKenzie D. Measurements of the elastic thickness under ancient lunar terrain. Icarus, 2005, 173: 100-107.
  • 8McKenzie D. Estimating Te in the presence of internal loads. J. Geophys. Res., 2003, 108(B9):2438.
  • 9Wieczoreck M A, Phillips R J. The structure and compensation of the lunar highland crust. J. Geophys. Res. , 1997,102:10933-10944.
  • 10Thomson D J. Spectrum estimation and harmonic analysis. Proc. IEEE, 1982,70:1055- 1096.

共引文献39

同被引文献39

引证文献4

二级引证文献9

相关作者

内容加载中请稍等...

相关机构

内容加载中请稍等...

相关主题

内容加载中请稍等...

浏览历史

内容加载中请稍等...
;
使用帮助 返回顶部