找出最主要的控矿因素,建立三因控矿分析思路   总被引：5，自引：3，他引：2  

高浩中  蔡新平 《地质与勘探》1998,34(5):1-2

通过几个已知金矿区的研究,认为到不同矿区有不同的控矿因素,首先找出最主要的控矿因素,再配合两个深层相关因素,进行矿体定位。  相似文献   

Prediction of the sawing quality of Marmarit stones using the capability of artificial neural network     

Hassan Yarmohamadi Samani  Ali Reza Yarahmadi Bafghi 《国际地质力学数值与分析法杂志》2012,36(7):881-891

The sawing rate is one of the most significant and effective parameters in extracting building stones via diamond wire sawing. This parameter designates the capability of diamond wire sawing for sawing different stones; in addition, the parameter gives rise to economical considerations for quarry designers. In this study, the existent relations between stone geotechnical parameters and the sawing rate of stones via diamond wire sawing were analyzed using regression and correlation coefficient as well as the collected data from Marmarit stone quarries. Moreover, we estimated the sawing rate of Marmarit using the dimensional stone rock mass rating (DSRMR); upon comparison of the data obtained from DSRMR our pre‐collected data on quarries, we did not gain satisfactory results from DSRMR, hence we used artificial neural network (ANN). The results showed that the percentage of Silica, the coefficient of water absorption, the uniaxial compressive strength (UCS), and abrasive hardness are the proper parameters for creating the ANN. Discontinuities have the least effects possible on diamond wire sawing. Having given the training possibility of the ANN, and its ability to evaluate relations among input parameters, the ANN, which was being trained with Marmarit's traits, was an accurate network for estimating diamond wire sawing in Marmarit quarries, although it could not generalize this network for other stones such as Chini and Crystal. Copyright © 2011 John Wiley & Sons, Ltd.  相似文献   

Multiscale approach to geo‐composite cellular structures subjected to rock impacts     

François Nicot  Philippe Gotteland  David Bertrand  Stéphane Lambert 《国际地质力学数值与分析法杂志》2007,31(13):1477-1515

Geo‐composite cellular structures are an efficient technological solution for various applications in civil engineering. This type of structure is particularly well adapted to resisting rockfalls and can act as a defensive structure. However, the design of such structures is for the most part empirically based; this lack of research‐based design stagnates optimization and advanced development. In this paper, the mechanical behaviour of a geo‐composite cellular structure is investigated using a multi‐scale approach, from the individual cell made up of an assembly of rocky particles contained in a wire netting cage to the entire structure composed of a regular array of cells. Based on discrete modelling of both the cell and structure scales, a computational tool has been developed for design purposes. Copyright © 2007 John Wiley & Sons, Ltd.  相似文献   

基于主成分分析的库存管理神经网络模型研究     

张欣 《广东海洋大学学报》2007,27(3):100-102

从影响合理库存的诸多因素中,利用数理统计的思想,找出若干主要指标,通过建立神经网络模型,进行模拟仿真,寻求一种解决问题的有效方法,把库存调整到理想的状态。  相似文献   

The Dependence of the Geoeffectiveness of Interplanetary Flux Rope on Its Orientation,with Possible Application to Geomagnetic Storm Prediction     

Yuming Wang  Pinzhong Ye  S. Wang 《Solar physics》2007,240(2):373-386

Interplanetary magnetic clouds (MCs) are one of the main sources of large non-recurrent geomagnetic storms. With the aid of a force-free flux rope model, the dependence of the intensity of geomagnetic activity (indicated by Dst index) on the axial orientation (denoted by θ and φ in GSE coordinates) of the magnetic cloud is analyzed theoretically. The distribution of the Dst values in the (θ, φ) plane is calculated by changing the axial orientation for various cases. It is concluded that (i) geomagnetic storms tend to occur in the region of θ<0°, especially in the region of θ≲−45°, where larger geomagnetic activity could be created; (ii) the intensity of geomagnetic activity varies more strongly with θ than with φ; (iii) when the parameters B ₀ (the magnetic field strength at the flux rope axis), R ₀ (the radius of the flux rope), or V (the bulk speed) increase, or |D| (the shortest distance between the flux rope axis and the x-axis in GSE coordinates) decreases, a flux rope not only can increase the intensity of geomagnetic activity, but also is more likely to create a storm, however the variation of n (the density) only has a little effect on the intensity; (iv) the most efficient orientation (MEO) in which a flux rope can cause the largest geomagnetic activity appears at φ∼0° or ∼ 180°, and some value of θ which depends mainly on D; (v) the minimum Dst value that could be caused by a flux rope is the most sensitive to changes in B ₀ and V of the flux rope, and for a stronger and/or faster MC, a wider range of orientations will be geoeffective. Further, through analyzing 20 MC-caused moderate to large geomagnetic storms during 1998 – 2003, a long-term prediction of MC-caused geomagnetic storms on the basis of the flux rope model is proposed and assessed. The comparison between the theoretical results and the observations shows that there is a close linear correlation between the estimated and observed minimum Dst values. This suggests that using the ideal flux rope to predict practical MC-caused geomagnetic storms is applicable. The possibility of the long-term prediction of MC-caused geomagnetic storms is discussed briefly.  相似文献   

基于土地利用的三维景观格局指数变化分析     

刘国栋  陈炜吉 《地理空间信息》2021,19(1):71-73,98

由于传统二维景观格局指数未考虑地形特征对景观格局指数的影响,为进一步研究地形结构对景观格局指数的影响,以重庆主城区为研究对象,利用ENVI5.2、ArcGIS10.5、Fragstats4.2平台,对重庆主城区不同城市化阶段的Landsat影像数据进行土地利用变化和三维景观格局分析。结果表明,2008-2018年研究区土地利用面积发生了较大变化,表现为林地和建设用地增加,耕地减少,湖泊与河流面积变化不大;景观格局变化主要表现为景观受人类干扰较强,随着城镇规划越来越合理,景观破碎度减少,景观异质性降低。通过对比二维景观格局指数发现,三维景观格局指数更能反映研究区的景观格局。  相似文献   

Chemical spots on the surface of the strongly magnetic Herbig Ae star HD 101412     

S. P. Jrvinen  S. Hubrig  M. Schller  I. Ilyin  T. A. Carroll  H. Korhonen 《Astronomische Nachrichten》2016,337(3):329-338

Due to the knowledge of the rotation period and the presence of a rather strong surface magnetic field, the sharp‐lined young Herbig Ae star HD 101412 with a rotation period of 42 d has become one of the most well‐studied targets among the Herbig Ae stars. High‐resolution HARPS polarimetric spectra of HD 101412 were recently obtained on seven different epochs. Our study of the spectral variability over the part of the rotation cycle covered by HARPS observations reveals that the line profiles of the elements Mg, Si, Ca, Ti, Cr, Mn, Fe, and Sr are clearly variable while He exhibits variability that is opposite to the behaviour of the other elements studied. Since classical Ap stars usually show a relationship between the magnetic field geometry and the distribution of element spots, we used in our magnetic field measurements different line samples belonging to the three elements with the most numerous spectral lines, Ti, Cr, and Fe. Over the time interval covered by the available spectra, the longitudinal magnetic field changes sign from negative to positive polarity. The distribution of field values obtained using Ti, Cr, and Fe lines is, however, completely different compared to the magnetic field values determined in previous low‐resolution FORS 2 measurements, where hydrogen Balmer lines are the main contributors to the magnetic field measurements, indicating the presence of concentration of the studied iron‐peak elements in the region of the magnetic equator. Further, we discuss the potential role of contamination by the surrounding warm circumstellar matter in the appearance of Zeeman features obtained using Ti lines. (© 2016 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Finding the most variable stars in the Orion Belt with the All Sky Automated Survey     

J.A. Caballero  M. Cornide  E. de Castro 《Astronomische Nachrichten》2010,331(3):257-273

We look for high‐amplitude variable young stars in the open clusters and associations of the Orion Belt. We use public data from the ASAS‐3 Photometric V ‐band Catalogue of the All Sky Automated Survey, infrared photometry from the 2MASS and IRAS catalogues, proper motions, and the Aladin sky atlas to obtain a list of the most variable stars in a survey area of side 5° centred on the bright star Alnilam (ε Ori) in the centre of the Orion Belt. We identify 32 highly variable stars, of which 16 had not been reported to vary before. They are mostly variable young stars and candidates (16) and background giants (8), but there are also field cataclysmic variables, contact binaries, and eclipsing binary candidates. Of the young stars, which typically are active Herbig Ae/Be and T Tauri stars with Hα emission and infrared flux excess, we discover four new variables and confirm the variability status of another two. Some of them belong to the well known σ Orionis cluster. Besides, six of the eight giants are new variables, and three are new periodic variables (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

苏丹穆格莱德盆地福拉凹陷油气成藏特征及勘探启示     

何碧竹  汪望泉  吕延仓 《现代地质》2010,24(4)

福拉凹陷下白垩统Abu Gabra组发育有湖相好—极好烃源岩,但热演化程度低、成藏主控因素不确定,勘探潜力不明。通过地层层序划分、构造分析、沉积相分析,认为张剪性区域构造背景控制福拉凹陷的构造与沉积发育,下白垩统Abu Gabra组发育有一定规模有效生烃凹陷,可形成Abu Gabra组烃源岩层,Abu Gabra组自储自盖,Bentiu组储、Aradeiba组盖及Aradeiba组自储自盖等3套生储盖组合,其中第二套储盖组合为该凹陷不同于六区其他凹陷的良好储盖组合。紧邻生烃凹陷、继承性发育的构造带,如中部滚动背斜—断鼻、南部次凹西缘断鼻、南部断阶带断鼻、北部次凹东缘断鼻等构造带是有利的成藏带。继承性发育的Fula1号滚动背斜、Fula2号断鼻构造具有多套储盖组合,勘探风险低,为有利的勘探目标。这些认识为福拉凹陷油气勘探提供了科学依据,且其研究方法及思路也为新区油气勘探提供良好的借鉴。  相似文献   

四川盆地南部下三叠统飞仙关组一段台内鲕滩的主控因素   总被引：2，自引：0，他引：2  

谭秀成  牟晓慧  罗冰  刘宏  刘晓光  丁熊  吴晓庆  吴兴波 《古地理学报》2010,12(1):49-55

四川盆地飞仙关组台缘鲕滩气田的发现,激励了人们重新认识台内鲕滩的发育分布规律及其勘探前景。根据野外露头及钻孔资料的分析,认为四川盆地南部飞仙关组一段的台内鲕滩具有发育向上变浅序列、单滩体厚度一般小于3m、横向连续性较差的特征。着重分析了沉积期古地貌、古水深、海水动荡程度以及古海平面相对升降变化对台内鲕滩的控制作用,并把滩体的发育阶段分为雏滩期(低速建造期)、滩核期(高建造期)及衰亡期3个阶段。结果表明,在缓慢等效的海退过程中,处于高能沉积界面附近的水下古高地有利于台内鲕滩的形成,继承性的泸州古隆起核部是区内有利的滩体发育区,形成的台内滩体具有一定的厚度规模和较大的分布面积。这一认识可为该区飞仙关组台内鲕滩的下一步勘探提供必要的地质支持。  相似文献