结合遥感数据与地统计学方法的海岸线超分辨率制图

使用黄河三角洲海岸Landsat卫星遥感数据,基于研究区域低分辨率6波段的海陆类型软分类结果及其变差函数,以高分辨率8波段的指示变差函数为精细尺度先验信息模型,采用数据探索性分析、协同指示克里格和序贯指示协同模拟技术,生成海陆类型发生概率模拟图像,通过等值线法提取海岸线空间分布特征。实验表明,基于地统计学方法的超分辨率制图技术在低分辨率遥感数据中融合高分辨率空间结构先验模型,可以较好表达精细尺度上的海岸线空间分布特征,同时保持原始数据的海陆类型组分信息及其空间结构特征。地统计学方法集成多尺度乃至多源空间信息的潜力通过海岸线超分辨率制图形式得到展示。     

全球灾害系统(GHS)在地质灾害预测预报中的简介

洪水和滑坡是两种典型的地质灾害。针对这两种地质灾害的预报预测,本文简介了全球灾害系统(GHS)及一些应用。基于遥感和预测模型集成的全球洪水和滑坡灾害的解决思路,笔者采用美国宇航局(NASA)集成的准实时卫星降雨的洪水模型和滑坡模型,初步开发成全球灾害系统(GHS)对相关地区进行研究。通过在洪都拉斯、印度尼西亚、中国汶川等实例研究,表明GHS在在大型洪水的时间和强度上具有较好的预测能力,同时,能较精确地预报出滑坡发生的时间和范围。最后本文提出该系统在福建省应用的展望。     

Three-dimensional Rayleigh hysteresis of oriented core samples from the German Continental Deep Drilling Program: susceptibility tensor, Rayleigh tensor, three-dimensional Rayleigh law

Rayleigh hysteresis, as defined by the well-known Rayleigh relations, has been observed not only when magnetization of pyrrhotite-bearing KTB-samples is measured in parallel to a weak dc magnetic field, but also in experiments where field and measuring directions have been adjusted strictly perpendicularly to each other. Nine-tupels of independent Rayleigh hysteresis loops could thus be compiled. Their characteristic coefficients X ^ijk of initial susceptibility together with the Rayleigh loss coefficients α^jk have been proved to determine completely the samples' weak-field magnetic anisotropy. Interpreting the coefficient matrices ( X ^ijk) and (α^jk) as the tensor of initial susceptibility and the Rayleigh tensor, respectively, generalization of the isotropic Rayleigh relations in terms of corresponding tensor relationships has been suggested for the anisotropic case. Application to the KTB samples showed 3-D Rayleigh hysteresis measurements to be an excellent tool for rock magnetic analysis in terms of ore content and crystalline texture. In particular, a magnetocrystalline double texture of the basal planes of pyrrhotite precipitates and their [1120] directions of easy magnetization have been clearly detected. Surprisingly, the welt-known theorem α= const. X ²_I, formulated by Néel (1942) for the isotropic case, has been found to hold true even in tensor generalization (α_jk) = const ( X ²_jk). To reach sufficient resolution for the measurements performed, a sensitive vibrating coil magnetometer (VCM) has been developed.     

心象地图在制图传输中的作用

制图传输是制图学的重要研究领域。本文从认知制图的角度,探讨了心象地图在制图传输中的作用;着重分析了心象地图和地图之间的内在联系,指出了人的认知制图能力的客观存在是制图传输得以进行的真正原因;在此基础上,提出了制图传输的扩展模式,增加了从读图者到次读图者之间的传输过程,并从内容和形式等方面分析了它的特殊性,以期完善制图传输模式。     

USE OF VALUE FUNCTIONS AS A POSSIBLE SUITABILITY SCALING PROCEDURE IN AUTOMATED COMPOSITE MAPPING

The application of composite suitability mapping integrated with a geographic information system is progressing at a much faster rate than the methodological improvements necessary for optimal use in the public planning context. The use of value functions is suggested as an alternative scaling procedure that is scientifically and operationally preferable to existing procedures. Value functions limit the operational subjectivity and enhance the potential for replication and verification of the analysis. Value functions are conducive to increased automation of the land planning and decision process while being comprehensible to non-expert decision-makers and the public.     

内力线定性描绘应力场方法及其在地质构造研究中的应用

为了简化地质构造力学分析，本文探讨了用内力线来描绘应力场的方法，仿照用磁力线描绘磁场的做法，约定以从外力作用点，支承点等处发出的一族主应力迹线为代表内力传递路径的“内力线”，根据弹性理论绘制了部分简单应力场的内力线图，阐述了以简单应力场内力线图为基础绘制复杂应力场内力线图并对之进行分析的方法，同时，文中还对这一方法在山字型构造体系和断裂等板内构造应力场分析，隐伏或未知构及地质的推测，地震预报等方面的应用做了尝试。     

佛山市顺德区飞鹅山Ⅲ号滑坡形成机理与防治技术

采用工程地质钻探、物探、地质测绘及室内试验等技术方法探讨飞鹅山Ⅲ号滑坡形成机理与防治技术。结果表明：1）滑坡体主要岩性为泥质粉砂岩,飞鹅山滑坡属于新形成的深层中型牵引式滑坡,在平面上呈圈椅状。2）滑坡属于双层滑面滑坡,主滑面以中型深层滑坡为主,主滑体上部发育中型中厚层滑坡。3）滑坡产生的原因为：(1)泥质粉砂岩倾向与坡向基本一致,且岩层倾角为中等倾角;(2)人工开挖使坡脚形成高陡临空面,抗滑力大为降低;(3)雨水沿层面及节理裂隙入渗至坡体深部,大大增加岩土体容重,同时泥质粉砂岩遇水软化,抗剪强度显著降低。4）结合该滑坡区地质环境条件,采用坡面削坡+锚杆（索）+格构梁+双排预应力锚拉抗滑桩+三维网植草绿化+截排水+毛石挡墙的综合治理方法进行防治,监测结果显示该滑坡变形及位移已得到有效控制,整治效果良好。     

Effects of magnetic interactions in anisotropy of magnetic susceptibility: Models, experiments and implications for igneous rock fabrics quantification

Besides granites of the ilmenite series, in which the anisotropy of magnetic susceptibility (AMS) is mainly controlled by paramagnetic minerals, the AMS of igneous rocks is commonly interpreted as the result of the shape-preferred orientation of unequant ferromagnetic grains. In a few instances, the anisotropy due to the distribution of ferromagnetic grains, irrespective of their shape, has also been proposed as an important AMS source. Former analytical models that consider infinite geometry of identical and uniformly magnetized and coaxial particles confirm that shape fabric may be overcome by dipolar contributions if neighboring grains are close enough to each other to magnetically interact. On these bases we present and experimentally validate a two-grain macroscopic numerical model in which each grain carries its own magnetic anisotropy, volume, orientation and location in space. Compared with analytical predictions and available experiments, our results allow to list and quantify the factors that affect the effects of magnetic interactions. In particular, we discuss the effects of (i) the infinite geometry used in the analytical models, (ii) the intrinsic shape anisotropy of the grains, (iii) the relative orientation in space of the grains, and (iv) the spatial distribution of grains with a particular focus on the inter-grain distance distribution. Using documented case studies, these findings are summarized and discussed in the framework of the generalized total AMS tensor recently introduced by Cañon-Tapia (Cañon-Tapia, E., 2001. Factors affecting the relative importance of shape and distribution anisotropy in rocks: theory and experiments. Tectonophysics, 340, 117–131.). The most important result of our work is that analytical models far overestimate the role of magnetic interaction in rock fabric quantification. Considering natural rocks as an assemblage of interacting and non-interacting grains, and that the effects of interaction are reduced by (i) the finite geometry of the interacting clusters, (ii) the relative orientation between interacting grains, (iii) their heterogeneity in orientation, shape and bulk susceptibility, and (iv) their inter-distance distribution, we reconcile analytical models and experiments with real case studies that minimize the role of magnetic interaction onto the measured AMS. Limitations of our results are discussed and guidelines are provided for the use of AMS in geological interpretation of igneous rock fabrics where magnetic interactions are likely to occur.     

东北平原杜蒙钻孔的磁性地层学和磁化率对松嫩古湖演化的指示

湖相沉积是过去气候环境变化研究的重要地质记录.东北平原在早-中更新世时期曾发育一个巨型湖泊(松嫩古湖), 对这一古湖的演化历史和机制仍需多钻孔的进一步研究.本研究针对东北平原杜蒙(HL)钻孔沉积物开展了²⁶Al/¹⁰Be同位素年代学、古地磁年代学、磁化率地层学和岩石磁学研究, 结果表明: (1)令字组和林甸组湖相沉积的界线为约900 ka; (2)林甸组的磁化率明显高于令字组, 令字组的高矫顽力弱磁性矿物贡献相对较大; (3)林甸组磁化率的升高可能与湖平面降低、水动力增强、入湖的强磁性矿物增多或者氧化还原条件改变, 从而生成了强磁性铁的硫化物有关; (4)约900 ka前后, 松嫩古湖萎缩, 可能与中更新世气候转型期间大西洋深层翻转流(Atlantic meridional overturning circulation, 简称AMOC)减弱致使热带辐合带(Intertropical Convergence Zone, 简称ITCZ)南移, 以及海平面下降造成更多陆地暴露地表, 水汽输送距离增加, 进而共同导致东亚夏季风降水减少有关.

     

黄土高原表土磁化率与气候要素的定量关系研究

黄土高原地区已建立多个表土低频磁化率-气候转换函数,为黄土古气候定量重建提供了关键方法。但是表土磁化率变化的气候控制因素的系统研究尚未开展; 同时,低频磁化率部分受到沉积作用的影响,需要寻找气候意义更明确的指标。我们系统采集了黄土高原及周边地区的表土样品,运用相关、回归和因子分析等方法,研究了不同气候要素及其季节变化对表土磁化率和频率磁化率的控制作用。结果显示,湿度是控制黄土高原表土磁化率的主要因素,温度的影响相对较小; 降水的季节分配也有影响,月降水变率较小的地区磁化率较高。在此基础上,选择反映成壤磁性颗粒组分的频率磁化率,建立了频率磁化率-年均降水量的转换函数,为黄土古气候定量估算提供了新的途径。