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Chen Wei Pradhan Biswajeet Li Shaojun Shahabi Himan Rizeei Hossein Mojaddadi Hou Enke Wang Shengquan 《Natural Resources Research》2019,28(4):1239-1258
Natural Resources Research - Groundwater is a vital water source in the rural and urban areas of developing and developed nations. In this study, a novel hybrid integration approach of... 相似文献
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Wei Chen Wenping Li Enke Hou Zhou Zhao Niandong Deng Hanying Bai Danzhi Wang 《Arabian Journal of Geosciences》2014,7(11):4499-4511
The main objective of this study was to apply a statistical (information value) model using geographic information system (GIS) to the Chencang District of Baoji, China. Landslide locations within the study area were identified using reports and aerial photographs, and a field survey. A total of 120 landslides were mapped, of which 84 (70 %) were randomly selected for building the landslide susceptibility model. The remaining 36 (30 %) were used for model validation. We considered a total of 10 potential factors that predispose an area to a landslide for the landslide susceptibility mapping. These included slope degree, altitude, slope aspect, plan curvature, geomorphology, distance from faults, lithology, land use, mean annual rainfall, and peak ground acceleration. Following an analysis of these factors, a landslide susceptibility map was produced using the information value model with GIS. The resulting landslide susceptibility index was divided into five classes (very high, high, moderate, low, and very low) using the natural breaks method. The corresponding distribution area percentages were 29.22, 25.14, 15.66, 15.60, and 14.38 %, respectively. Finally, landslide locations were used to validate the results of the landslide susceptibility map using areas under the curve (AUC). The AUC plot showed that the susceptibility map had a success rate of 81.79 % and a prediction accuracy of 82.95 %. Based on the results of the AUC evaluation, the landslide susceptibility map produced using the information value model exhibited good performance. 相似文献
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On the study of the basic characteristics of geological objects and the special requirement for computing 3D geological model, this paper gives an object-oriented 3D topologic data model. In this model, the geological objects are divided into four object classes: point, line, area and volume. The volume class is further divided into four subclasses: the composite volume, the complex volume, the simple volume and the component. Twelve kinds of topological relations and the related data structures are designed for the geological objects. 相似文献
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HOUEnke WULixin WUYuhua JUTianyi 《地球空间信息科学学报》2005,8(2):122-127
On the study of the basic characteristics of geological objects and the special requirement for computing 3D geological model, this paper gives an object-oriented 3D topologic data model. In this model, the geological objects are divided into four object classes: point, line, area and volume. The volume class is further divided into four subclasses., the composite volume, the complex volume, the simple volume and the component. Twelve kinds of topological relations and the related data structures are designed for the geological objects. 相似文献
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面向地质建模的三维体元拓扑数据模型研究 总被引：27，自引：0，他引：27
在对地质对象的基本特征和计算机三维地质建模的基本要求进行讨论的基础上，提出了面向对象的三维体元拓扑数据模型。在该数据模型中，用面向对象的方法将地质对象抽象为点、线、面、体，体类又进一步划分为复合体、复杂体、简单体和体元四类。对所有对象类设计了12种拓扑关系和相应的数据结构。 相似文献
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三维地学模拟几个方面的研究现状与发展趋势 总被引：27，自引：0，他引：27
对三维地学模拟中的三维空间数据模型,三维地学模拟技术以及三维地学模拟软件的应用３个方面的研究现状进行了总结,并指出了发展趋势与研究思路。 相似文献
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Harry Enke Matthias Steinmetz Hans-Martin Adorf Alexander Beck-Ratzka Frank Breitling Thomas Brüsemeister Arthur Carlson Torsten Ensslin Mikael Högqvist Iliya Nickelt Thomas Radke Alexander Reinefeld Angelika Reiser Tobias Scholl Rainer Spurzem Jürgen Steinacker Wolfgang Voges Joachim Wambsganß Steve White 《New Astronomy》2011,16(2):79-93
We present status and results of AstroGrid-D, a joint effort of astrophysicists and computer scientists to employ grid technology for scientific applications. AstroGrid-D provides access to a network of distributed machines with a set of commands as well as software interfaces. It allows simple use of computer and storage facilities and to schedule or monitor compute tasks and data management. It is based on the Globus Toolkit middleware (GT4).Chapter 1 describes the context which led to the demand for advanced software solutions in Astrophysics, and we state the goals of the project.We then present characteristic astrophysical applications that have been implemented on AstroGrid-D in chapter 2. We describe simulations of different complexity, compute-intensive calculations running on multiple sites (Section 2.1), and advanced applications for specific scientific purposes (Section 2.2), such as a connection to robotic telescopes (Section 2.2.3). We can show from these examples how grid execution improves e.g. the scientific workflow.Chapter 3 explains the software tools and services that we adapted or newly developed. Section 3.1 is focused on the administrative aspects of the infrastructure, to manage users and monitor activity. Section 3.2 characterises the central components of our architecture: The AstroGrid-D information service to collect and store metadata, a file management system, the data management system, and a job manager for automatic submission of compute tasks.We summarise the successfully established infrastructure in chapter 4, concluding with our future plans to establish AstroGrid-D as a platform of modern e-Astronomy. 相似文献
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Paula G. Benavidez Daniel D. Durda Brian L. Enke William F. Bottke David Nesvorný Derek C. Richardson Erik Asphaug William J. Merline 《Icarus》2012,219(1):57-76
Collisions are a fundamental process in the creation of asteroid families and in satellite formation. For this reason, understanding the outcome of impacts is fundamental to the accurate modeling of the formation and evolution of such systems. Smoothed-Particle Hydrodynamics/N-body codes have become the techniques of choice to study large-scale impact outcomes, including both the fragmentation of the parent body and the gravitational interactions between fragments. It is now possible to apply this technique to targets with either monolithic or rubble-pile internal structures. In this paper we apply these numerical techniques to rubble-pile targets, extending previous investigations by Durda et al. (Durda, D.D., Bottke, W.F., Enke, B.L., Merline, W.J., Asphaug, E., Richardson, D.C., Leinhardt, Z.M. [2004]. Icarus 170, 243–257; Durda, D.D., Bottke, W.F., Nesvorný, D., Enke, B.L., Merline, W.J., Asphaug, E., Richardson, D.C. [2007]. Icarus 186, 498–516). The goals are to study asteroid–satellite formation and the morphology of the size–frequency distributions (SFDs) from 175 impact simulations covering a range of collision speeds, impact angles, and impactor sizes. Our results show that low-energy impacts into rubble-pile and monolithic targets produce different features in the resulting SFDs and that these are potentially diagnostic of the initial conditions for the impact and the internal structure of the parent bodies of asteroid families. In contrast, super-catastrophic events (i.e., high-energy impacts with large specific impact energy) result in SFDs that are similar to each other. We also find that rubble-pile targets are less efficient in producing satellites than their monolithic counterparts. However, some features, such as the secondary-to-primary diameter ratio and the relative separation of components in binary systems, are similar for these two different internal structures of parent bodies. 相似文献
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宁夏羊场湾煤矿浅埋煤层开采地面塌陷发育规律及形成机理 总被引：1，自引：0，他引：1
以宁夏羊场湾煤矿Y110207工作面为研究对象,采用无人机遥感技术、野外调查与有限差分软件模拟方法研究浅埋煤层开采的地面塌陷类型、发育规律及其形成机理。(1)浅埋煤层开采地面塌陷以地表裂缝发育为主,地表破坏严重。(2)平行切眼裂缝间隔性出现,展布于整个工作面内,间隔距离为10～120m,局部裂缝形成错台高度约为15cm。平行顺槽裂缝为拉张型裂缝,发育在顺槽至外围一定范围。(3)采煤活动导致地下形成采空区,上覆岩层发生移动破坏,破坏区分为剪切破坏区、拉张破坏区及剪-拉破坏区,分别对压应力区、拉应力区和压-拉转化区。(4)当应力扰动传递至地表,应力值超过覆盖层抗拉强度时地表产生裂缝。随着工作面推进,覆岩内部裂缝带上行裂缝与地表下行裂缝贯通,形成错台。研究成果丰富了该区浅埋煤层的地面塌陷理论知识,为地面塌陷防治提供了理论依据。 相似文献