向下延拓在深部矿产勘探中的应用——以青海某矿区为例

勘测深部盲矿体时,矿体距离观测点较远,磁异常的相互叠加常常在地面形成具有一个磁异常中心的宽缓磁异常,分辨不清矿致异常和背景异常。通常用向上延拓、方向导数等处理的效果差强人意。笔者采用向下延拓方法处理了青海某矿区的宽缓磁异常,向下延拓深度为30倍点距,获得了精细的各矿体异常特征。通过与大量的见矿、未见矿钻孔比较,向下延拓场反映的磁异常位置与已见矿钻孔有较好的对应关系,同时指示出全部的未见矿钻孔都处于向下延拓场反映的磁异常外围。基于当前向下延拓方法的稳定计算问题已经取得突破,笔者认为针对一些大埋藏深度的宽缓磁异常采用向下延拓处理,区分叠加异常,圈定异常位置,可以获得事半功倍的效果,为钻孔布置提供佐证。同时对勘探精度也作了一些有意义的讨论。     

Detection of Hg pollution by stream sediment geochemistry in the Bisagno valley (Genoa, Italy)

 Systematic stream sediment investigation in a periurban area surrounding Genoa (Italy) revealed the existence of a significant mercury anomaly localized on the main (3rd rank) bed of the Bisagno river. Statistical multivariate analysis of elemental abundances points out the anthropic nature of this contamination. Because of the well-known bioaccumulation of Hg in contaminated media, attention must be focused on the risks associated with the discovered pollution. Received: 30 November 1999 · Accepted: 22 March 2000     

Arsenic as an indicator element for gold exploration in the region of the Xiangxi Au–Sb–W deposit, NW Hunan, PR China

The Xiangxi Au–Sb–W deposit, the largest of its type in northwestern Hunan, China, is a sulfide-dominated ore body hosted by low grade metamorphic red slates of the Neoproterozoic Madiyi Formation. Three stages of mineralization, quartz–scheelite, quartz–gold–pyrite, quartz–gold–stibnite, and one metal-barren stage of veining, quartz–calcite, are recognized. Arsenopyrite occurs only as a minor mineral phase in the second stage. Analyses for 21 trace elements show that the enrichment factors of As in the metal deposit (EC [=element concentration of sample/average content of an element in the upper crust]: 190; 43 samples) in ore veins and in the Guanzhuang and Yuershan reference sections (3.7 km and 2.7 km away from the Xiangxi mine, EC: 3.5; 96 samples) are much smaller than those of Sb (52855 [in ore veins], 117 [in the sections]), W (5665, 7.5) and Au (2727, 5.3). The background concentrations of Au and As in the two sections were 1.4 ppb and 1.4 ppm, respectively. Arsenic (with an anomaly coefficient [AC = number of anomalous samples/total number of samples] of 76%) forms a larger geochemical halo than W (AC: 8%) and Au (AC: 32%). Gold and As in the deposit were transported mainly as metal complexes such as Au(HS)⁻₂, H_nAs₃S⁻⁽³⁻ⁿ⁾₆ (n=1, 2 or 3) and HAsS⁰₂. Au(HS)⁻₂ is rapidly precipitated by a geochemical oxidation barrier — the red slates of the Madiyi Formation. As–S complexes in the stratigraphic horizon can be transformed into As–O complexes (e.g., H₃AsO⁰₃) under oxidizing conditions, and are continuously transported. Therefore, they can be widely distributed in the red slate units, thus forming extensive geochemical haloes, so that As can be used as an indicator element for Au exploration in the Xiangxi region.     

贵州省1：200000区域化探数据入库及检索应用

本文是一份数据入库方法及检索应用的总结。文中主要介绍了利用计算机进行化探数据入库及检索应用。入库数据可进行标准图幅检索、任意区域检索等多条件数据检索，检索出的数据可作多种化探数据处理，并绘制等值线图、色块图等图形及图像。此项技术经济投入少，能及时检索数据、处理数据、显示及打印图形、图像，以指导找矿及勘探，具有一定的实用价值。     

大姚、民乐-山丹地震前的中短期前兆

利用川滇及青藏块体北缘地区上世纪80年代至2003年的跨断层流动形变观测资料，借助应变强度比时序曲线，通过丽江Ms7．0、景泰Ms5．9等震例研究，获取与2003年7月大姚Ms6．2、Ms6．1地震和10月民乐-山丹Ms6．1地震孕育有关的中短期前兆异常。分析表明：①大姚、民乐-山丹地震前1年内异常场地数远超过场地总数的1／3，相对近源区异常在发震地区占一半；②大姚Ms6．2地震前半年内，盐源-丽江地块及其邻近区域以及北东向延伸的川滇交界地区异常明显增多，相对集中。2003年7～9月大幅减弱；而鲜水河断裂、楚雄-通海断裂南段有所增强；③民乐-山丹震前十余天至数月内相对近源区及其邻近构造区域呈现异常相对分散-相对集中且局部增强-一临震前减弱的时空演变特征。震后一个月内青藏块体北缘地区仍有近1／3的场地呈现异常(海原一六盘山断裂带尤为突出)。     

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Scientific field training for human planetary exploration

Forthcoming human planetary exploration will require increased scientific return (both in real time and post-mission), longer surface stays, greater geographical coverage, longer and more frequent EVAs, and more operational complexities than during the Apollo missions. As such, there is a need to shift the nature of astronauts’ scientific capabilities to something akin to an experienced terrestrial field scientist. To achieve this aim, the authors present a case that astronaut training should include an Apollo-style curriculum based on traditional field school experiences, as well as full immersion in field science programs. Herein we propose four Learning Design Principles (LDPs) focused on optimizing astronaut learning in field science settings. The LDPs are as follows:

(1)

LDP#1: Provide multiple experiences: varied field science activities will hone astronauts’ abilities to adapt to novel scientific opportunities

(2)

LDP#2: Focus on the learner: fostering intrinsic motivation will orient astronauts towards continuous informal learning and a quest for mastery

(3)

LDP#3: Provide a relevant experience—the field site: field sites that share features with future planetary missions will increase the likelihood that astronauts will successfully transfer learning

(4)

LDP#4: Provide a social learning experience—the field science team and their activities: ensuring the field team includes members of varying levels of experience engaged in opportunities for discourse and joint problem solving will facilitate astronauts’ abilities to think and perform like a field scientist.

The proposed training program focuses on the intellectual and technical aspects of field science, as well as the cognitive manner in which field scientists experience, observe and synthesize their environment. The goal of the latter is to help astronauts develop the thought patterns and mechanics of an effective field scientist, thereby providing a broader base of experience and expertise than could be achieved from field school alone. This will enhance their ability to execute, explore and adapt as in-field situations require.     

The invention that opened the solar system to exploration

The invention of gravity-propelled interplanetary space travel (also known as “gravity-assist trajectories”) in the early 1960s broke the high-energy barrier of classical space travel based on reaction propulsion, and made possible the exploration of the entire solar system with instrumented spacecraft. In this concept, a free-fall spacecraft is launched from a launch planet P₁ to a nearby planet P₂ such that its gravitational field (superimposed on the gravitational field of the Sun) catapults the vehicle to another planet P₃, which in turn is used to repeat the process. Thus, through a series of planetary encounters, a gravity-propelled trajectory P₁-P₂-P₃-P₄-…-P_N is generated. This paper describes how the invention was conceived and how the difficult mathematical problem of computing the trajectories was solved in order to numerically investigate and use the invention in actual missions. The crucial roles played by the UCLA Computing Facility and the Departments of Mathematics and Physics are also described.     

大陆深部地壳物质成分识别方法综述

本文系统总结了大陆深部地壳物质成分识别研究方法和元素丰度合理性检验的方法,以期为大陆深部地壳物质成分探测提供技术方法体系。深部地壳物质成分识别的主要方法有:①因构造运动抬升出露到地表的中下地壳剖面;②地表出露的高级变质地体;③产于火山岩中的深部地壳捕掳体,如麻粒岩捕掳体;④地球物理测深资料与深部岩石物理性质的高温高压实验测定结果之间的拟合和⑤壳源岩浆岩源区地球化学示踪。元素丰度合理性检验的方法主要有地表热流和元素比值法。     

可控源音频大地电磁法深部找矿实验效果

为了考查电磁法在探测深部金属矿及地质构造方面的实际效果,用可控源音频大地电磁法分别在埋深为500 m和1 100 m的两个已知隐伏铁、铜矿体上进行了实验工作。实验结果表明地电异常显示了矿体、断层以及岩层接触带的分布。在矿体埋藏深度小于500 m、矿层较厚时,地电异常十分明显;若矿体埋藏深度大于1 000 m,地电异常主要反应了控矿、容矿构造。