空间点面拓扑关系不确定性的模糊描述研究

阐述空间数据和空间关系不确定性的概念、来源及建模,并研究利用模糊理论进行空间区域的划分,以及利用模糊九交模型对空间对象拓扑关系进行描述分析.     

BHαBAR: big Hα kinematical sample of barred spiral galaxies – I. Fabry–Perot observations of 21 galaxies

We present the Hα gas kinematics of 21 representative barred spiral galaxies belonging to the BHαBAR sample. The galaxies were observed with FaNTOmM, a Fabry–Perot integral-field spectrometer, on three different telescopes. The three-dimensional data cubes were processed through a robust pipeline with the aim of providing the most homogeneous and accurate data set possible useful for further analysis. The data cubes were spatially binned to a constant signal-to-noise ratio, typically around 7. Maps of the monochromatic Hα emission line and of the velocity field were generated and the kinematical parameters were derived for the whole sample using tilted-ring models. The photometrical and kinematical parameters (position angle of the major axis, inclination, systemic velocity and kinematical centre) are in relative good agreement, except perhaps for the later-type spirals.     

五台山绿岩带金矿的Pb同位素地质演化

五台山绿岩带中各种类型金矿化是地壳演化不同阶段的产物，在成矿作用和矿质来源诸方面均存在着明显的区别。而这些，完全可以通过矿物和岩石普通Pb同位素的组成、构造-化学模式和同位素示踪等分析而获得可靠的依据。     

庐山运动

本文简述了庐山隆-滑构造的基本特征。在中元古代双桥山群底部的顺层韧变带中，把前人的断层构造砾或沉积成因的巨厚层状变质复成分砾岩，自上而下分离出三层砾：上部砾、中部砾、下部砾。其中上部砾为断层构造砾；中部砾不是砾，而是构造分泌物；下部砾为沉积底砾。在此基础上，同时参考研究区早元古代星子群与中元古代双桥山群构造、岩浆活动、变质作用等方面的差异，建立了“庐山运动”，其活动时间为2200～1800Ma，这可以与华北及华南其它地区同时期的构造运动相对比，但庐山运动的强度相对较弱，表现为以垂直隆升为特色的造陆运动，它曾使研究区早元古代晚期至少遭受过长达200Ma（1800～1600Ma）的风化、剥蚀作用。     

Kinematics and Dynamics of Galaxies in Compact Groups for a sample of 31 groups

A long-term program based on Fabry-Perot Hα velocity field data of compact groups has been undertaken in order to analyse the kinematics of the compact group galaxies and the extent of their dark halos. The data are taken at the ESO and the CFH 3.6 m telescopes. The main goals of our project are: • To determine the evolutionary stages of the studied groups, • To search for tidal dwarf galaxy candidates in heavily interacting systems and • in combination with photometry available in the literature, to determine the Tully-Fisher relation for the group galaxies. The sample contains examples of groups at a variety of dynamical stages: from a false group that is in fact one single irregular galaxy with several star-forming blobs (e.g. H18) to a group whose members are strongly interacting and possibly forming tidal dwarf galaxies (e.g. H92) to a group in the final process of merging. We have so far identified five HCG classes: 1. merging groups2. strongly interacting, 3. weakly interacting, 4. non-groups, 5. single irregular galaxies. The ones which can be used in the TF studies are those in classes (2) and (3), for which comprehensive rotation curves can be derived. This revised version was published online in September 2006 with corrections to the Cover Date.     

山西省五台山—恒山地区脉状金矿成矿的地球动力学

０　前　言（代序）该文集命名为“成矿的地球动力学”,表明它只是矿床学中一项较基础性的研究;把脉状金矿作为研究对象,则应属于金矿区域成矿学的范畴。展望２１世纪,资源、环境乃是人类生存与发展之本,因此矿床学所肩负的使命必将更加艰巨。虽然人类利用矿产资源已有数千年的历史,但作为地质科学的重要组成部分—矿床学到１６世纪中叶才萌芽,１９世纪才形成具有较完整理论的学科。如果说矿床学的基本任务是确定这种或那种矿床在地壳中的生成条件和分布规律,矿床的形成又非孤立和偶然的事件,它是一定地质构造背景和地质历史条件下…     

联合InSAR与无人机航测的白鹤滩库区蓄水前地灾隐患广域识别

白鹤滩水电站位于我国西南高陡山区,是我国实施“西电东送”的国家重大工程之一。水库两岸是地质灾害高易发区,传统的地质灾害调查手段存在工作效率低、危险性高、无法覆盖高位隐患点等弊端。联合星载合成孔径雷达干涉测量技术(InSAR)与无人机航测技术应用于广域地灾隐患探测对于库区地灾隐患广域识别、掌握其分布规律及辅助后续重点防治具有重要意义。本文基于142景Sentinel-1卫星升降轨影像,采用时间序列InSAR技术对白鹤滩库区重点库岸段蓄水前两岸活动性坡体进行探测,同时利用无人机航测技术对其进行了野外验证与辅助分析,根据航片生成的数字高程模型(DEM)、数字正射影像图(DOM)、三维模型等航摄数字产品,结合形变与地形地貌特征,确定了32处地灾隐患点。并结合隐患点的形变量级、形变面积、是否涉水、是否具有明确威胁对象等因素给出了防治建议,建立了全面而准确的蓄水前地灾隐患灾害库。最后基于此案例对两种技术优势特长、适用范围以及如何高效联合应用进行了总结。本文揭示了两种技术在广域地灾隐患识别时的结合应用,无人机航测不仅能对InSAR技术探测到的形变区进行验证,同时InSAR也可以指导重点航测区域,提高航测飞行效率。通过结合两项技术提供的实时与历史信息、形变与地质信息可实现综合研判,形成基于空天遥感技术的高效库岸地质灾害综合遥感识别方法。