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非球形轴对称粒子光散射的散射矩阵元素展开系数的数值计算

扼要地介绍了非球形粒子光散射的散射矩阵元素按广义球函数展开的基本理论,以及球形粒子散射矩阵元素间的关系。在此基础上较详细地阐述了计算展开系数的方法以及在程序研制中所遇到的一些问题。最后,对非球形的Ｃｈｅｂｙｓｈｅｖ粒子光散射的散射矩阵元素的展开系数进行了计算,结果表明数值技术和计算的正确性。     

ALCGEIS知识获取与推理机设计

运用专家系统的知识获取和推理机设计原理与方法,探讨了ALCGEIS系统的基本结构、知识分级、知识获取过程和实现程序,推理机的基本原理和控制策略及其程序实现的算法,以及推理知识的搜索策略;论述了 AIEGEIS推理规则的设计方法及其推理算法。     

地球物理学中的电磁场正演与反演

本文在近年来众多的地球物理研究者的研究基础上,总结了当前地电磁模型正反演已有成果,定量分析了各种主要正反演的性能测试,指出不同正反演法的优点、缺点以及应用范围局限,提出了各种方法的发展趋势以及当前计算地球物理领域的核心内容,指出了计算地球物理领域的数值模拟发展方向.     

前陆盆地挠曲沉降正演模型的设计与实现——以库车古近纪陆内前陆坳陷沉降分析为例

本文以二维薄板弹性挠曲模型为基础,对模型进行简化和参数优化选取,并在VC++6.0环境下采用Windows视窗设计,实现了前陆盆地挠曲沉降的正演模拟系统.应用这一系统模拟分析了库车古近纪-新近纪前陆盆地的挠曲沉降过程.模拟结果表明,库车古近纪-新近纪前陆盆地的沉降曲线总体呈上凸型,具有典型前陆盆地沉降的特点,根据沉降速率变化可以把整个沉降过程分为四个部分,分别对应盆地的四个构造层序发育阶段,每一阶段呈不同的沉降特征,相邻两阶段之间存在一盆地回弹隆升、逆冲构造活动终止期,盆地遭受广泛剥蚀形成两个构造层序之间的不整合界面.正演模拟通过将沉降过程时间离散,精细设定不同时间段的构造负载,能够精细恢复前陆盆地的沉降过程和演化.     

大气中一类非线性方程的非线性波解及周期的近似计算法

大气中许多模式可化为Ｆ＇＇＝ＡＦ／Ｆ＋Ｂ（ＡＢ≠０）一类非线性常微分方程。利用常微分方程定性理论说明了该方程存在非线性波解，讨论了其周期的计算问题，并求得了波解及其周期的近似表达式。     

利用原生岩浆定量反演原岩微量元素丰度的方法

利用同源不同程度平衡部分熔融作用形成的两种原生岩浆岩的微量元素浓度，提出了一种定量反演原岩微量元素丰度的方法。反演前不需要做任何人为假设，为定量研究源区的微量元素地球化学提供了一个有力的手段。对汉诺坝新生代橄榄拉斑玄武岩和碱性玄武岩的成因及地幔源区特征作了讨论。反演结果显示本区地幔相对球粒陨石有过明显的ＲＥＥ富集过程，并且不同的ＲＥＥ富集程度存在显著的差异。     

Study of the crust and mantle using magnetic surveys by Magsat and other satellites

Among the first measurements made from near-Earth orbiting satellites were measurements of the magnetic field. The sources of that field lie both within the Earth, in its core and crust, and in the surrounding ionosphere and magnetosphere. This article summarizes some of the methodology and results for studies of the Earth’s mantle and crust. Mantle conductivity studies can be made either by studying signals impressed on the Earth from outside, e.g., the ionosphere or magnetosphere, or by studying signals originating in the core and transmitted through the mantle. Crustal field studies begin with a careful selection of the data and subsequent removal of core and external fields by some sort of filtering. Average maps from different local times sometimes differ, presumably due to the remaining presence of fields of external origin. Several techniques for further filtering are discussed. Where large-area aeromagnetic maps are available, crustal maps derived from satellite data can be compared with upward continued data. In general, the comparisons show agreement, with some differences, particularly in and near the auroral belts. The satellite data are further reduced by various methods of inverse and forward modelling, sometimes including reduction to the pole (RTP). These techniques are generally unstable at the equator. Common methods of stabilizing the inversions include principle components analysis and ridge regression. Because of the presence of the core field, the entire crustal contribution from the field is not known. Also, there is a basic nonuniqueness to the inverse solutions. Nevertheless, magnetizations that are interpretable can be derived.