IMPLICIT NONLINEAR NORMAL MODE INITIALIZATION:A MULTIGRID APPROACH

The implicit nonlinear normal mode initialization (INMI) is applied to a tropical limited area shallow water modelin spherical coordinates.The boundary condition for the INMI scheme is based on the boundary formulation of themodel.The INMI scheme is found to be very efficient in suppressing spurious gravity wave oscillation and providing awell balanced initial data set for the model.The INMI scheme involves solving a number of elliptic type equations withvarying complexity.and hence an efficient numerical technique is required for solving such equations.In order to makeINMI computationally more attractive,we are employing the multigrid method for solving all the elliptic type equationsin the INMI scheme.The numerical procedures for the development of such multigrid solvers are briefly described.     

中国西北地区剪切波三维速度结构

本文研究区包括中国西北地区几个不同的构造单元,即准噶尔、阿尔泰、天山、内蒙古褶皱、塔里木盆地、柴达木和祁连山地区.从群速度和剪切波速度模型上可以看出,除塔里木具有十分明显的稳定构造体特征外,其它地区均具构造活动地区的特征,但其速度表现各具特点,并与它们的构造演化史有关.莫霍界面的起伏基本上控制了布格重力异常的分布;另外,天山地区与北山的速度结构在土地幔盖层中差别很大,天山的上地幔高速盖层可能与应力场有关.     

湖北大别山区土地资源生产力估算

本文以湖北大别山区为例,提出了自然条件复杂,资料缺乏的山区土地资源第一性生产力的估算方法,并计算了湖北大别山区土地资源的生产力。即在土地资源带及类型(组合)区划分的基础上,以资源类型(组合)区为基本单元,通过典型地区抽样获取资料,运用多种数学模型测算,并经过综合判定,求得各类型(组合)区,资源带主要作物的第一性生产力。     

闽粤台沿海北西西向最新构造带与大震构造背景

闽粤台沿海自台湾运动以来逐渐形成了多条北西西向隆起—拗陷的最新活动构造带,与已知的北东—北北东向隆起、拗陷带构成了区域性镶嵌构造格局。 研究区内除板块相互碰撞、俯冲及上地幔物质上涌形成大震构造背景外,莫霍面隆起或隆起断距大、低速层厚、地壳变薄、近两、三千年地表抬升差异活动显著以及台东近海有北西西向构造活动等,也都是发生大震的重要构造背景     

大庙斜长岩同位素地质年龄、稀土地球化学及其地质意义

大庙斜长岩的⁴⁰Ar/³⁹Ar年龄测定呈现出一条典型的马鞍型年龄谱,在中温阶段有二个明显的坪年龄1656±15 Ma和1029±7 Ma,结合其构造位置和全球斜长岩分布来看,它们分别代表了侵位年龄和后期热扰动的时代。密云奥长环斑花岗岩中角闪石的⁴⁰Ar/³⁹Ar坪年龄为1716±21 Ma。两者时空上密切相关,代表了裂谷作用初期非造山环境中双模式岩浆作用产物。斜长岩类和苏长岩之间稀土配分模式的相似性表明,它们明显为同一成因的岩浆分异系列的产物。     

吉林省夹皮沟金矿地质特征及成因探讨

夹皮沟金矿产于晚太古宙绿岩带的下部层位。北西向的韧性剪切带控制着金矿田和矿床分布,而矿体主要受叠加于韧性剪切带之上的脆性断裂构造制约。金主要来源于围岩。华力西晚期—燕山早期为主要成矿期。属多源、多期的叠生型金矿床。     

陕西地区岩浆岩Nd、Sr同位素特征及其与大地构造发展的联系

岩浆岩Nd、Sr同位素特征表明,扬子地块基底有着和华北地块很不相同的早期演变历史。这意味着华北和扬子两地块在历史上曾经是相互独立的,后来才拼合在一起。Nd、Sr同位素研究还表明,华北和扬子两地块的会聚在泥盆纪以前就已经在进行中,它是通过位於两地块之间的古秦岭海洋壳俯冲消亡在华北地块之下实现;华北和扬子两陆块最终相碰撞至少发生在二叠纪以前。     

苏皖凹凸棒石矿物红外光谱特征研究

苏皖凹凸捧石粘土矿物包括沉积、风化及火山碎屑蚀变三种成因类型。成矿物质来源于内陆浅水湖盆水下玄武岩风化蚀变及地表玄武岩的风化。不同成因类型的凹凸棒石在矿物晶体结晶程度上有较大差异。通常,由风化作用生成并与碳酸盐共生的沉积型凹凸棒石结晶程度低,较纯的并与硅质岩共生的沉积型凹凸棒石结晶程度高。它们在红外吸收光谱特征上表现为:前者红外振动吸收带分裂程度低,吸收峰弱且峰形钝。后者红外振动吸收带分裂程度高,吸收峰尖锐。因此研究凹凸捧石的红外吸收光谱特征可基本上区分出它们的成因类型。本文还对凹凸棒石红外吸收光谱振动波数带进行了划分,并对相应的振动类型作了探讨。     

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.     

Palaeomagnetism and rock magnetism of the Deccan traps

Extensive work on the palaeomagnetism of the Deccan traps by several workers has revealed only one reversal (normal-reverse-normal) of the geomagnetic field during the period of eruption of these flows. The scatter in the natural remanent magnetic directions of different flows in a sequence of these traps is rather large and it persists even after magnetic cleaning. Generally this large scatter of directions is attributed to the geomagnetic secular variation during formation of the traps. Recent studies of the magnetic properties of the trap samples indicate that the presence of multidomain magnetite in a lava sequence differs from locality to locality in the Deccan trap province and so the stability of their natural remanent magnetization. While these features can be clearly perceived, an understanding of the same seems to be quite difficult. However, it appears that part of the scatter in directions could be due to the alteration of the magnetic minerals in the Deccan traps and hence it would not be proper to relate the entire scatter to the secular variation.