Contrasting morphodynamics in alluvial fans and fan deltas: effect of the downstream boundary

Alluvial fans and fan deltas can, in principle, have exactly the same upstream conditions, but fan deltas by definition have ponding water at their downstream boundary. This ponding creates effects on the autogenic behaviour of fan deltas, such as backwater adaptation, mouth bars and backward sedimentation, whereas alluvial fans may lack these effects. Hence the present authors hypothesize that morphodynamics on alluvial fans are determined primarily by upstream boundary conditions, whereas morphodynamics on fan deltas are determined by both the upstream and the downstream boundary condition and changes therein. To isolate the effects of the upstream and downstream boundaries, five new alluvial fan experiments are compared with the details of three fan deltas published earlier that were formed under very similar and simple conditions. Similar to the fan deltas, the alluvial fans build up by sheet flow, whilst quasi‐regular periods of incision cause temporary channelized flow. Incision is followed by channel backfilling, after which the fan returns to sheet flow. The channelization and backfilling in alluvial fans is markedly less pronounced and more prone to autogenic disturbance than in fan deltas. The difference is caused by morphodynamics at the downstream boundary. In a fan delta, the flow expansion of the channel causes deposition of all the sediment, which forms a mouth bar and causes strong backfilling. In an alluvial fan, on the other hand, the slope break at the fan perimeter causes some deposition, but transport is not reduced to zero. Consequently, the backfilling in alluvial fans is less pronounced than in fan deltas. Other published experiments support this trend: removal of the mouth bar by a river leads to permanent channelization, whilst pronounced mouth‐bar formation in highly channelized deltas promotes backward sedimentation. The experimental results for this study predict that, when alluvial fans prograde into lakes or deep rivers, they transition to fan deltas with increasingly deeper channels and thicker backfill deposits.     

高产高效矿井地质条件的定量预测与检验模型

提出地质等性块段法与模糊综合评判法相结合评价煤层开采地质条件的方法对评价指标系统、验证指标系统、指标值赋值及合成,权系数和算子选定,评价方法及评价结果的验证,评价工作流程作了阐述,通过实例证明该方法客观可靠,有推广价值。     

复杂地质条件下组合围堰施工

在复杂的地质条件下,根据现场地质情况选择合理的围堰成为深基坑开挖过程中支护与止水的关键。结合柳州双拥大桥22号墩主塔基础施工,介绍了采用锁口钢管桩与钢筋混凝土支护桩相结合的组合围堰来进行复杂地质条件下的围堰施工技术。     

陕西省铝土矿地质特征及成矿规律

陕西省已知铝土矿产地主要分布于陕北的府谷县、渭北的铜川-韩城一带和陕南的西乡、镇巴、南郑地区;已知铝土矿都位于沉积间断面上,受地层层位控制,属滨海-浅海相沉积矿床。陕北和渭北铝土矿主要产于石炭系下统下部本溪组,陕南铝土矿主要产于二叠系上统吴家坪组底部王坡页岩段。成矿的地质构造条件是隆起区边缘。成矿物质来源既有基底碳酸盐岩的溶蚀分解物,也有陆源铝硅酸盐岩的风化分解物。气候条件是有利于使岩石中铝质析出的温暖潮湿条件。时间上有一个较长时间的沉积问断。对成矿有利的地形条件是古地形总体比较平缓,有利于铝硅酸盐风化物在缓慢的搬运过程中充分分解析出Al2O3。     

降雨作用下山区边坡稳定性分析

降雨是诱发边坡失稳破坏的主要原因,本文以坡地水文模型为基础,结合无限边坡稳定计算模型,研究降雨条件下边坡启动的临界降雨条件。通过工程算例表明:降雨量与边坡体稳定系数成反比;滑坡启动的临界降雨量随边坡坡度的增大而减少;随边坡土体内摩擦角的增加而逐渐增加,此分析对降雨型滑坡的研究有借鉴性的意义。     

浙西北淳安银山地区银铅锌矿床矿石结构构造、矿石成分及成矿机制

浙西北与同处钦杭成矿带东段的赣东北和皖南相比,由于其地质研究程度较低,在该区尚未能找到大型多金属矿床。近年来,随着地质勘查程度的不断提高,淳安地区银山一带发现中型以上银铅锌矿床。本文选取银山矿区钻井岩芯中富含银、铅、锌矿石样品,利用显微镜观察和电子探针分析等方法,对其中的银等多金属的矿石结构构造、矿石成分及成矿机制等进行了较深入的研究。研究表明,银山地区多金属(银、铅、锌)矿体主要分布在蓝田组上段与上覆皮园村组之间的接触带中,另有部分处于蓝田组层内岩性变化的界面以及蓝田组底部白云质灰岩和下伏南沱组含砾泥岩之间,均呈似层状展布。矿石呈自形-半自形粒状结构、他形粒状结构和交代残余结构以及块状构造、浸染状构造和网脉状构造。金属矿物组合主要分为黄铁矿-黄铜矿-方铅矿-闪锌矿和磁黄铁矿-毒砂-闪锌矿两组,其中前者位于蓝田组顶部和皮园村组之间,属于中低温热液型的矿物组合,后者位于蓝田组下部和南沱组之间,属于中温热液型的矿物组合。通过对不同金属矿物中银含量的对比分析,得出银山地区银元素主要赋存在方铅矿中。脉石矿物有石英、方解石、白云母、绿泥石、单斜辉石等,尤其在矿石中多见的细粒单斜辉石按其成分上的差异分为透辉石和钙铁辉石两类,指示了热液作用对成矿的显著影响。综上所述,笔者认为浙西北银山多金属矿床成因很可能为早期层控-后期中低温热液改造的叠生型矿床。其形成机制是:震旦纪时期海相火山喷流沉积使得部分多金属成层聚集,蓝田组地层为银山多金属矿床的形成提供了部分的物质来源,加里东期的变质变形作用及其发育的断裂构造也具有一定的控制作用;随后,大规模的燕山期花岗质岩浆及其流体组分沿断裂带上侵,不仅使得原有地层中的多金属元素进一步富集,而且其本身也可能带入部分多金属流体,从而使得富含多金属元素热液流体在具有地球化学障的岩性界面上富集成矿。此项研究对该地区及邻区进一步找矿勘探具有重要的科学意义和应用价值。     

红外热成像在龙门石窟奉先寺渗水探测中的应用

奉先寺是龙门石窟具有代表性的作品之一。石窟岩性为碳酸盐岩,渗水病害严重威胁着岩体和雕刻品的完整性。准确探测出渗水部位和渗水来源等是奉先寺渗水治理方案设计的重要依据。利用红外热成像技术,在不同条件下对奉先寺崖壁渗水进行现场探测。结果表明,使用热成像仪可以准确有效地探测出崖壁岩体的渗水部位,判断出渗水来源、分布及其活动规律。与以往依靠人工观察相比,红外热成像技术有着明显的优势。该技术可在石窟渗水勘察中应用推广。     

Reviews on Potash Deposit Metallogenic Conditions

Potash salt is one of key scarce strategic resources. Searching for large scale of potash salt deposit is one big problerm which Chinese academic community faces. Many new discoveries of world potash deposit have been made in recent ten years, which provide abundant practical information and complement the potash metallogenic theory. Through the summary of the potash forming characteristics at home and abroad, the paper studies the potash forming time, tectonic condition, paleogeographic condition, paleoclimate, basin location and salt source. Potash is mainly formed in Permian, Cretaceous, late Jurassic, Cambrian and Devonian. The combination of structure and environment helps to form large scale of evaporation. The climate cycle is related with crust activity. As the other ore deposit, the formation of potash ore also needs dry climate. Potash is the product of final stage in brine evolution, and therefore, it needs persistent drought climate. However, the climate condition is very complicated. Drought climate belt also occurs in humid climate stage, which is controlled by geomorphology. Potash ore can also form in local drought condition. Generally, potash forms in rock salt basin. However, the actual situation is very complicated. Some potash basin is coincided with rock salt basin, some is on one side of rock salt basin; and some are even in the outside of rock salt basin. Salt materials can be from three sources: marine source, terrigenous source and deep source.The paper gives an overview of the research status about the potash deposit forming conditions, which has great guiding significance for searching potash deposit in China. The paper also summarizes the three types of metallogenic models for potash deposit, including epicontinental metallogenic model, abnormal marine evaporation model and rift valley model. The three models are mainly different in material sources, in which the potash in epicontinental metallogenic model is from seawater; the potash in abnormal evaporation model is from nonmarine brine and the potash in rift valley model is mainly from deep material of volcanic activity.     

黑龙江乱泥沟金矿成矿条件与找矿方向

乱泥沟矿区第四系砂金矿产丰富，是寻找岩金的有利靶区。区内出露的古元古代变质岩系地层的原岩为泥质粉砂岩和中基性海底火山岩，其Au含量高，是金矿成矿的初始矿源层。区内NE，NW向构造发育，所发现的矿体均受控于NW向断裂，呈脉和复脉状产于构造蚀变带及其次一级的层间破碎带中，成矿物质简单，矿体品位和厚度变化系数较小，为中—低温蚀变岩型金矿床。利用物化探测量手段，圈出具找矿意义的组合异常，通过工程查证发现金矿体。在综合研究矿区地质特征及物化探异常的基础上总结了找矿标志，并指出下一步有利的找矿区段。     

云南省白竹箐-阳文山NE向构造带铅锌矿成矿地质条件及找矿方向

重点分析构造带的成矿地质条件，总结地层、构造、岩浆岩与矿床的关系，认为该地区具有寻找层控及热液改造型铅锌矿的远景，并指明找矿方向，根据化探异常及矿点分布的规律，圈定了找矿靶区。