斑岩铜矿中铂族元素的研究现状及展望

文章对当前国内外斑岩铜矿中铂族元素的研究现状进行了较为详细的阐述，指出研究与铂族元素矿化有关的斑岩铜矿的流体包裹体及其富集成矿过程，以及铂族元素对斑岩铜矿成矿环境，成岩岩浆的起源和成矿物质来源示踪是该领域的发展方向和前沿。     

土屋-延东斑岩型铜(钼)矿床多源信息找矿模型

为提高东天山铜镍成矿带内的矿产勘查效益，文章综合了区域成矿环境、矿床特征、地球物理场、地球化学场等成矿信息，尝试建立了土屋—延东斑岩型铜钼矿床的多源信息找矿模型。认为成矿带内铜矿资源远景良好，必将成为我国又一个铜矿资源潜力区。     

豫西寨凹斑岩型铜矿地质特征及其成矿远景

据寨凹铜矿的大地构造背景、控矿构造、成矿母岩、成矿元素分带、蚀变等特征，该铜矿属斑岩型铜矿。寨凹地区地球物理、地球化学、遥感、成矿母岩和构造条件对成矿十分有利，有形成大中型斑岩型铜（银金）矿的资源潜力。     

福建上杭铜矿沟—萝卜岭斑岩型铜矿床地质特征及远景评价

上杭县铜矿沟和萝卜岭矿段组成一个斑岩型铜矿床．萝卜岭矿段位于花岗闪长斑岩北东端的前峰部位，铜矿沟则是其往南西深部的延伸，通过对铜矿沟—箩卜岭斑岩型铜矿床地质特征的研究，认为铜矿沟斑岩型铜矿埋藏总体较浅、品位较低、厚度稳定且较厚，对于指导该区寻找浅部斑岩型铜矿具有重要的意义。     

西藏驱龙斑岩铜钼矿地球化学异常特征

驱龙铜矿发育多元素的岩石地球化学异常.成矿元素Cu、Mo、(Ag)异常强、规模大,异常与矿化区一致;伴生元素Au、Bi、Pb、As、Sb、Hg异常在Cu、Mo异常边部并套合产出的B Co、Ni Mn Zn的异常主要分布铜钼矿化带外侧.Na₂O在矿化区显示负异常,K₂O为正异常.从异常元素组合、水平分带性和贫Na₂O、富K₂O的成矿环境表明,矿床属典型的斑岩型铜矿地球化学特征,并受到了强烈的剥蚀.     

砂岩岩脉(岩墙、岩床)的一种可能成因——冲蚀沟槽的充填

黄河三角洲的边滩、心滩上发育了大量冲蚀沟槽（冲槽）．这些冲蚀沟槽深数厘米至1m～2m，宽数厘米至数米，长数十厘米至十几、二十余米，但以深数十厘米，宽数厘米至十余厘米，长数米者多见。形态多样，有直立板片状、直立楔状、“⊥”状、梯形状、“U”形状及树枝状等，其内有时被风成砂充填。经成岩作用后，它们便会转变成砂岩岩脉（岩墙、岩床）。因此，冲蚀沟槽的（砂）充填可能是一种砂岩岩脉（岩墙、岩床）的形成方式．     

多宝山超大型铜矿床的成矿构造环境

多宝山超大型铜矿床是我国典型的斑岩型矿床，主要产出于多宝山组岛弧建造和花岗闪长岩、花岗闪长斑岩中，成矿年龄为292～283Ma。根据地球物理异常及大量的基性和超基性岩体，以及通过对比两侧的岩石圈结构、古生物、结晶基底、成矿特征和地球化学特征，认为黑河一嫩江是一条重要的构造边界带，它是兴安和松嫩地块在早石炭世拼合、碰撞、造山隆起形成的。多宝山超大型铜矿床就是形成于两板块碰撞后隆起抬升构造环境的斑岩型铜矿床。     

山东沂南金场矽卡岩型金铜矿床地质地球化学特征及矿床成因

金场金铜矿床是沂沐断裂带西侧与中生代次火山作用有关金铜矿床的典型代表。该矿地质地球化学特征的综合研究表明“其成矿岩体具有富碱、富钾、富轻稀土和大离子亲石元素的特点，是由成熟度较高的中－下部地壳物质经重熔再生的 产物。     

Metallogenic model of the copper deposit

The copper deposits in the mid-lower reaches of the Changjiang River consist mainly of porphyry, skarn and massive sulphide deposits. According to the geological background, the types of ore deposits and the mineralization, the metallogenic model of the copper deposits is discussed. It is pointed out that the ore-forming hydrothermal fluids came mainly from magmatic water and were related to the intermediate-acid intrusions, and that the formation of skarn arid massive sulphide deposits coincided with the mineralization of porphyry deposits. Project supported by Doctorate Foundation of the State Education Commission of China.     

Properties of wave velocity for two types of granitoids at high pressure and temperature and their geological meaning

The wave velocity for two types of granitoids was measured using the analytic method of full-wave vibration at high pressure and high temperature. The laws of velocity changes for them differ with the pressure boost and temperature rise, and the velocity change of S-type is more violent than that of I-type. The “softening point” of compressional wave velocity (V μ) is also revealed during the measurement for two types of granitoids imitating the pressure and temperature at a certain depth. But the depth of “softening”, V_p after “softening” and the percentage of V_p’s drop around the “sofrening point” for two types of granitoids are obviously different. The depth of “softening” is 15 km approximately and V_p after “softening” is 5.62 km/s for S-type granitoid. But for I-type granitoid the depth of “softening” is 26 km approximately and V_p after “softening” is 6. 08 km/s. Through careful analysis of rock slices after the experiment, it was found that the “softening” of elastic-wave velocity is caused by the partial melting of granite. Combined with the results of geophysical prospecting, these results suggest that the low-velocity layers developing in the interior of Earth crust are related to thc partial melting of different types of granitoids. The formation of the low-velocity layer in the upper-middle Earth crust is closely related to the development of S-type granitoid, but that in the lower Earth crust is closely related to the development of I-type granitoid.