新疆皮山镁质矽卡岩矿床(含糖玉)成因及锆石SHRIMP U-Pb定年

新疆且末—若羌一带的和田玉,以带有黄绿色调为特征,针对该种和田玉的颜色成因和特性表征研究较少,影响了对这种和田玉的颜色和矿床成因的认识。本文利用电子探针(EPMA)、背散射电子图像(BSE)、X射线荧光光谱(XRF)、高分辨电感耦合等离子体质谱(HR-ICP-MS)分析技术对且末黄口料的矿物组成和化学成分进行测试,采用滴定法测试FeO含量,探究其颜色成因和成矿类型,并采用锆石SHRIMP U-Pb同位素定年约束其成矿时代。结果表明：该地区和田玉主要由磷灰石、方解石、白云石、透辉石、绿帘石、榍石和锆石组成。其稀土总量低(∑REE=2.61~19.1μg/g),稀土配分模式呈现出明显Eu负异常(δ Eu < 0.05)、LREE右倾、HREE平坦,根据稀土配分模式和Cr、Ni元素含量,推测是一种镁质矽卡岩型和田玉。且末黄口料和田玉Fe³⁺/Fe²⁺平均值(0.16)与其他地区和田玉有重叠,但该比值稍高(0.07~0.26),而Fe³⁺、Fe²⁺含量与其他地区和田玉之间差异并不明显。因此,推测且末—若羌和田玉的颜色成因与Fe³⁺/Fe²⁺比值有关,与Fe³⁺、Fe²⁺含量并无明显关系; 该地区和田玉中锆石SHRIMP U-Pb同位素定年获得的两个加权平均年龄为461.7±6.1Ma (MSWD=1.6)和498.1±4.6Ma (MSWD=1.16),代表了该地区黄绿色和田玉的形成时代,并可以进一步约束西昆仑的构造演化。

     

江西冷水坑银铅锌矿田构造地球化学的若干问题

本文重点对冷水坑银铅锌矿田构造发育特征和构造地球化学的若干问题进行了初步探讨。运用裂隙统计、显微构造和组构分析方法对矿田NE向、NW向和近EW向断裂的力学性质和活动方式作了概略性论述。研究了银路岭矿床三个构造地球化学剖面的分析结果,其中主要成矿元素和伴生元素的分布和丰度变化与构造发育的关系,显示出本区构造地球化学场具有一定的分布规律。矿田F_1断裂是有一定区域意义的重要的成岩成矿和控岩控矿断裂,本次工作中选择了茶田剖面对F_1断裂带构造地球化学特征进行了初步探讨。     

中国河南东秦岭—桐柏成矿区、带的划分

东秦岭桐柏区域成矿规律的研究,是以不同时期的板块或地体俯冲或碰撞增生构造分析为基础。根据华北地台南缘由两个早寒武地体所组成,划分出华熊成矿区和嵩箕成矿区。著名的秦岭—桐柏褶皱带即为秦岭—桐柏成矿带;而成矿亚带的划分是以不同时期活动陆缘增生或造山带为根据的,它们分别是中元古、加里东和海西成矿亚带。文中阐述了构造环境和成矿作用,并提出花岗岩类及其成矿作用板块构造模式,特别是中生代大储内都挤压或A—型俯冲的成岩成矿模式。     

中国滇西兰坪—思茅地洼盆地内中轴断裂带的初步研究

通过对中、新生代兰坪—思茅地洼盆地东、西部沉积特征、岩浆活动、地球物理场和卫星影像资料的综合研究与对比分析,论证了盆地内中轴断裂带的地质特征;讨论了中轴断裂带对盆地演化和成矿作用的重要意义。它是该区深部动力作用的主导构造 ,又是该区超大型、大型矿床形成的主要控制因素。     

青藏高原东缘—扬子特提斯构造域深部结构与地壳形变研究

青藏高原东缘和扬子西缘的构造带是中国特提斯构造域的重要组成部分,该构造域受欧亚板块与印度板块陆—陆碰撞、高原隆升、块体裂解或拼接挤压等强烈构造活动的影响,记录和保存了多期次的特提斯构造演化历史痕迹。同时,该研究区域也是中国西部地区地壳形变最强烈的地区之一,其浅表形变特征与深部构造之间存在怎样的关联和制约机制是目前国际地球科学的一个研究热点。本研究依据作者十多年来持续在该区域开展的地质—地球物理研究,通过深部地球物理多参数结构成像、沉积盆地分析、地壳形变和强震孕育机制等综合对比分析,发现在青藏高原东缘的下地壳存在低速和高泊松比异常带,该异常体与来自青藏高原上涌的软流圈热物质汇聚,导致从扬子西缘到青藏高原的下地壳和上地幔的深部结构发生显著变化。沿着龙门山断裂带,中、下地壳存在交叠相间的低速(高泊松比)和高速(低泊松比)区域,这些深部结构分布特征与地表形变及前陆盆地隆坳格局具有较好的一致性。基于上述认识,提出了青藏高原东缘—扬子板块的深部接触模式及其相应的盆山耦合关系,阐明了板块碰撞—耦合的深部动力学过程对剧烈地壳形变、盆地隆坳格局和强震诱发的制约关系。本研究成果将为深入认识青藏高原东缘高原急剧隆升、盆地基底结构与隆拗格局,以及强烈地壳形变的深部动力学机制提供参考信息。     

云县邦东—景谷民乐地区火山岩型铜矿找矿前景

本区位于滇西特提斯沟—弧—盆构造体系的主火山弧地体中,处于澜沧江褶断束东凸弧形转折处,上三叠统小定西组钙碱性火山碎屑岩、次火山岩含矿,火山机构控制矿体的产出形态,后期构造、侵入体使矿体叠加、富积,矿化类型为火山—次火山岩热液改造矿床;地、物、化、遥等成矿地质条件有利,具有很好的找矿前景。     

鸡西群城子河组时代的进一步探讨

近年来 ,古生物工作者在鸡西群城子河组及其相当地层的生物化石研究方面取得了巨大的进展。在总结这些新的材料的基础上 ,通过与国外的化石组合进行对比 ,从海相双壳类、植物、孢粉及海相沟鞭藻化石等多方面的证据 ,尤其是根据 Thracia rotundata、Vectianella、Pseudaphrodina ricordeana等欧洲 Aptian阶重要的双壳类化石、被子植物及三沟类被子植物花粉的出现 ,城子河组的时代应为 Aptian期 - Albian期早期     

Radio Properties of BL Lac Object S5 2007+777

S5 2007+777 is a typical BL Lac object with a low peak frequency, and a kpc-scale extended X-ray jet. In the literature, the Doppler factor derived at the X-ray waveband by means of model estimation is about 13.0, then the intrinsic jet scale can reach the order of magnitude of 1 Mpc. In this work, we have studied the radio structure of the jet, the brightness temperature, proper motion and other properties of this source with the collected EVN (European VLBI Network) high-resolution archive data, and the American VLBA (Very Long Baseline Array) 15 GHz observed data, etc. It is found that the jet directions measured at the different wavebands of the VLBI (Very Long Baseline Interferometry) are consistent, but slightly different from the direction of the kpc-scale X-ray jet given by the literature and the direction of the VLA (Very Large Array) radio jet, which means that the Doppler brightening effect exists in the jet emission of the source. Both the mean value and median value of the radio Doppler factor of this source estimated from the brightness temperature that measured by the VLBI are 5.0, which is smaller than the Doppler factor at the X-ray waveband given by the literature, but consistent with the Doppler factor at the radio waveband obtained by using the other methods in the literature. Furthermore, by fitting the data observed in multiple epochs, it is found that the various components of the source at the same waveband do not have an evident proper motion in a long epoch, but the proper motion in short epochs exhibits even a super-luminal motion. This may be caused by the transfer of the central position of the component with a low surface brightness. Meanwhile, this also verifies the conclusion that the radio Doppler factor estimated previously is not very large, and smaller than the Doppler factor in the X-ray waveband. By using the obtained radio Doppler factor, it is found that the source has an intrinsic radio jet of rather large scale, which may reach 0.5 Mpc, because the mean value is adopted in this case, thus it indicates that the source also possibly possesses a jet close to the scale of a giant radio galaxy.     

Reliability Analysis of Main-axis Control System of the Antarctic Equatorial Astronomical Telescope Based on Fault Tree

The Antarctic astronomical telescopes work chronically on the top of the unattended South Pole, and they have only one chance to maintain every year. Due to the complexity of the optical, mechanical, and electrical systems, the telescopes are hard to be maintained and need versatile expedition teams, which means that an excessive awareness is essential for the reliability of the Antarctic telescopes. Based on the fault mechanism and fault mode of the main-axis control system for the Antarctic equatorial astronomical telescope AST3-3 (Antarctic Schmidt Telescope 3-3), the method of fault tree analysis is introduced in this article, and we obtain the importance degree of the top event from the importance degree of the bottom event structure. From the above result, the hidden problems and weak links of the system can be effectively found out, which will indicate the direction for improving the stability of the system and optimizing the design of the system.