个旧锡矿阿西寨矿段化探异常分带及找矿意义

通过对个旧锡矿阿西寨矿段地表基岩的地球化学勘查。发现其成矿元素的地球化学异常表现出明显的环状分带，并以测区内隐伏花岗岩凸起为中心，元素分带序列与元素本身的地球化学性质所决定的侧向迁移活动能力相符合。该现象再次证实个旧锡矿为花岗岩岩浆期后热液成矿，花岗岩是大多数成矿金属元素的物质来源，同时也是成矿热液活动的主要驱动营力。分析认为，阿西寨测区是一个相对较完整和独立的(凸起)成矿场，成矿热液活动以阿西寨凸起为中心。成矿热液活动体系受断裂导流影响，在以花岗岩凸起为中心的分带控制下，可能存在的工业矿体将在主干断裂附近和有利的构造岩性界面产出。     

Gravity anomalies and associated tectonic features over the Indian Peninsular Shield and adjoining ocean basins

A combined gravity map over the Indian Peninsular Shield (IPS) and adjoining oceans brings out well the inter-relationships between the older tectonic features of the continent and the adjoining younger oceanic features. The NW–SE, NE–SW and N–S Precambrian trends of the IPS are reflected in the structural trends of the Arabian Sea and the Bay of Bengal suggesting their probable reactivation. The Simple Bouguer anomaly map shows consistent increase in gravity value from the continent to the deep ocean basins, which is attributed to isostatic compensation due to variations in the crustal thickness. A crustal density model computed along a profile across this region suggests a thick crust of 35–40 km under the continent, which reduces to 22/20–24 km under the Bay of Bengal with thick sediments of 8–10 km underlain by crustal layers of density 2720 and 2900/2840 kg/m³. Large crustal thickness and trends of the gravity anomalies may suggest a transitional crust in the Bay of Bengal up to 150–200 km from the east coast. The crustal thickness under the Laxmi ridge and east of it in the Arabian Sea is 20 and 14 km, respectively, with 5–6 km thick Tertiary and Mesozoic sediments separated by a thin layer of Deccan Trap. Crustal layers of densities 2750 and 2950 kg/m³ underlie sediments. The crustal density model in this part of the Arabian Sea (east of Laxmi ridge) and the structural trends similar to the Indian Peninsular Shield suggest a continent–ocean transitional crust (COTC). The COTC may represent down dropped and submerged parts of the Indian crust evolved at the time of break-up along the west coast of India and passage of Reunion hotspot over India during late Cretaceous. The crustal model under this part also shows an underplated lower crust and a low density upper mantle, extending over the continent across the west coast of India, which appears to be related to the Deccan volcanism. The crustal thickness under the western Arabian Sea (west of the Laxmi ridge) reduces to 8–9 km with crustal layers of densities 2650 and 2870 kg/m³ representing an oceanic crust.     

Slab behaviour and its surface expression: new insights from gravity modelling in the SE-Carpathians

We use lithosphere-scale gravity models to calculate gravity anomalies resulting from oceanic subduction, continental collision, slab steepening, delamination, and break-off. Local isostasy was assumed for determining vertical movements caused by mass changes related to these tectonic processes. Our results show that subduction is accompanied by basin subsidence on the upper plate caused by the heavy lithospheric root of the subducting slab. The basin evolution goes parallel with the slab evolution and shows considerable modifications when the processes at depth change (slab steepening, delamination, break-off). Characteristic gravity anomaly curves were acquired for the different tectonic scenarios. These curves together with other data (e.g. basin evolution on the upper and the lower plate) were used for the reconstruction of the tectonic evolution of the SE-Carpathians which includes Tertiary subduction and collision followed by slab steepening and delamination.     

引力位虚拟压缩恢复法

提出了一种将地球表面的引力位虚拟地压缩到地球内部的一个球体表面 ,进而求解在整个地球外部空间 (包括地球边界上 )的重力位场以及重力场的方法     

地球重力场与KBR系统频谱关系的建立与分析

以近极圆形轨道的SST-Ⅱ为研究目标，利用解析的方法分析卫星间精密测距与地球重力场的频谱关系，得出了一般情况下300km高度的SST，星间距离每增加100km，恢复能力提高约10阶次；对于500km卫星高度的SST，星间距离每增加100km，恢复能力提高约5阶次的结论。研究成果可以为我国发展SST探测地球重力场的卫星计划提供参考。     

用遗传算法反演地壳的变密度模型

用青藏高原布格重力异常资料 ,结合亚东 格尔木地学断面得到的Moho面结构 ,反演了青藏高原中部地壳内密度随深度变化的指数分布函数 ,试验得出地壳表层与地幔的密度差约为 - 0 .92 6 g·cm-3 ,地壳的平均密度值为 2 .75 0 g·cm-3 。     

利用现有重力场模型求定CHAMP卫星加速度计修正参数

CHAMP卫星加速度计数据的标定是通过确定其尺度因子和偏差参数来完成的.本文基于能量守恒方程,给出利用现有重力场模型标定CHAMP卫星加速度数据的基本原理和数学模型;提出相邻历元间差分算法,大大简化了观测方程,同时避免积分常量的计算.该算法既能同时解算尺度因子和偏差参数,也可任意求解其中之一.基于实测的CHAMP卫星加速度数据,利用EGM96模型和最新公布的EIGEN-2模型进行计算与比较,验证该方法的有效性.     

地球重力场、重力、重力梯度在三维直角坐标系中的表达式

现代卫星重力测量主要利用星载GPS接收机、加速度计、星载测距仪等来确定重力卫星的轨道 ,削弱非保守力的干扰 ,由此根据卫星的位置、速度及其变率来确定地球重力场。而上述GPS等星载仪器所提供的数据 ,包括卫星轨道坐标及其速率、扰动加速度、星间距离及其变率 ,都是以三维直角坐标 (x ,y ,z)的形式表示的 ,因此 ,地球重力场、重力和重力梯度在三维直角坐标系中的表达式在卫星重力解算中具有实际意义     

基于时空分析的贫困丘陵山区耕地变化机理研究

在地理信息系统技术的支持下 ,利用耕地面积变化时间序列模型、耕地动态度模型、耕地重心变化模型等 ,对湖北省咸宁市耕地的时间变化和空间变化特征进行了定量的研究 ,并应用主成分分析法 ,选择 2 3个因素对其驱动因子进行了相关分析。结果表明 ,耕地变化主要受经济因子、人口、房地产政策及耕地开发强度的影响