北部湾沉积物记录的近千年以来气候环境变化          下载免费PDF全文

林俊川  孔德明  陈法锦  黄超 《海洋学研究》2022,40(3):49-61

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Characteristics and tectonic setting of volcanic rocks in Early Cretaceous Baiyingaolao Formation of Keyouzhongqi area，Inner Mongolia   总被引：1，自引：0，他引：1  

KONG Yuanming  MA Rui  HE Zhonghua  YANG Deming  WU Qing  WANG Yang 《世界地质(英文版)》2014,17(2):78-85

The authors studied zircon LA-ICP-MS U-Pb dating,the zircon Hf isotope and geochemistry of acidic volcanic rocks in Baiyingaolao Formation of Keyouzhongqi area,Inner Mongolia,and discussed the chronology, source region and tectonic setting of the volcanic rocks in the studied area． The clear oscillatory zoning of zir- cons indicates a typical magmatic origin,and the results of dating show that the volcanic rocks of Baiyingaolao Formation were formed in Early Cretaceous (121.5 ±1.0 Ma)． The features of major and trace elements show that the rocks are alkali-rich,poor in calcium and magnesium with enrichment in LILEs like Th,U,K and Gd and depletion in HFSEs,e.g. Nb,Ta,Sr and Ti． The fact implies that they were the products of partial melting of the crust． εHf(t) = ( +6.30--+9.06) and TDM2=600--835 Ma,suggest the magma originated from par- tial melting of the young crust． Combined with the evolution of regional tectonic structure,the authors conclude that the acidic volcanic rocks of Baiyingaolao Formation may be formed under the extensional environment relat- ed to the subduction of Paleo-Pacific Plate．  相似文献   

Petrogenesis and tectonic setting of granite porphyry in Keyouzhongqi area,Inner Mongolia     

WU Qing  YANG Weihong  HE Zhonghua  YANG Deming  MA Rui  WANG Jianguo 《世界地质(英文版)》2014,17(1):24-33

The authors studied the geochemistry,zircon U-Pb ages,Hf isotope of the granite porphyry and its petrogenesis and tectonic setting in the studied area． The zircon U-Pb dating indicates the formation of the gran- ite porphyry is in Early Cretaceous (125． 1 ±1． 5 Ma)． The granite porphyry has high-SiO2and alkali-rich fea- tures,which belongs to high-K calc-alkaline series rocks (A/CNK = 0． 95%--1． 25%)． The analyses of trace elements show the characteristics of a swallow-shaped ＲEE distribution pattern with enrichment in LＲEEs and most of LILEs and HFSEs,depletion in Ba,Sr,Nb,P and Ti,and especially strong depletion in Eu,which indicates the granite porphyry belongs to the aluminous A-type granite． Their εHf(t)range from 5． 94 to 8． 80 with Hf two-stage model ages (TDM2) of 620 Ma to 803 Ma． Combining with the regional tectonic background, we conclude that the source of the rocks is the new crust materials accreted from depleted mantle in Neoprotero- zoic and is the product of partial melting of middle and lower crustal rocks,which may be suffered from the dual impact of the subduction of the Palaeo-Pacific Ocean and the closure of the Mongol-Okhotsk Ocean．  相似文献   

Reservoir characteristics and main controlling factors of oil sand in Houba area,northwestern Sichuan Basin,China   总被引：1，自引：0，他引：1  

Xuefei Yang  Xingzhi Wang  Shaonan Zhang  Hao Tang  Deming Zeng  Lin Xie 《Arabian Journal of Geosciences》2014,7(6):2119-2128

Houba oil sand in frontier Longmenshan Mountain is one of the most typically important unconventional resources. The basic reservoir characteristics of oil sand and the main factors affecting reservoir quality were examined in this article based on porosity, permeability, and mercury porosimetry measurements; thin section analyses; SEM observation; and X-ray diffraction analysis. This study shows that the oil-bearing sandstone reservoir is mainly medium?coarse-grained sublitharenite and litharenite. The main pore type is intergranular pores, including residual primary intergranular pores, dissolved intergranular pores, and dissolved intragranular pores; fractures are common in this study area. The quality of sandstone reservoir is of high porosity and high permeability with a high oil saturation of 89.84 %. It is indicated that the main controlling factors of the reservoir in the study area include deposition, diagenesis, and tectonism. Deposition laid a foundation to porosity evolution, and channel sand is the most favorable depositional facies for the reservoir. Diagenetic alterations are the keys to reservoir evolution; dissolution and chlorite coatings cementation play an effective role in the generation and preservation of pores. Compaction, carbonate cementation, and quartz overgrowth cause many damages to the reservoir porosity. Fractures caused by structural breakages can improve the reservoir permeability and they also can provide fluid migration pathways to the late corrosion, which formed a lot of corroded fissures as reservoir and percolation spaces.  相似文献   

西藏冈底斯南缘中新世含矿斑岩源区组成与成因     

高成  李德威  刘德民  罗文行  冯旻旻  李华亮 《大地构造与成矿学》2014,(4)

青藏高原南部中新世下地壳流动是当前大陆动力学研究的热点,关键科学问题是下地壳的流动方向。LA-ICP-MS定年结果表明冲江斑状黑云母二长花岗岩的形成时代为14.9~14.8 Ma,朱诺斑状花岗岩的形成时代为15.3~14.9 Ma。含矿埃达克质斑岩的特征如下:Si O2含量67.72%~74.49%,K2O含量2.85%~5.98%,Sr含量93~804μg/g,高Sr/Y(16~139)、(La/Yb)N(21~43)比值,Eu/Eu*值为0.6~0.91。冲江岩体锆石εHf(t)值为1.2~5.1,朱诺岩体锆石εHf(t)值为–6.9~–0.1,他们与徐旺春等报道的镁铁质麻粒岩的锆石Hf值(–2.5~4.8)具有很好的叠合性,暗示镁铁质麻粒岩(印度镁铁质下地壳)可以作为他们的岩浆源区。此外,Sr-Nd同位素表现出雅鲁藏布江蛇绿岩和拉萨地块两个端元混合的特征,Pb同位素表现出雅鲁藏布江蛇绿岩和喜马拉雅富集陆壳端元的特征。上述同位素地球化学特征表明,冈底斯中新世埃达克质斑岩的岩浆源区物质组成包括:拉萨陆壳、印度陆壳、雅鲁藏布江蛇绿岩(地幔成分),表现出加厚下地壳部分熔融特征,暗示青藏高原南部由南向北的下地壳流动方向。  相似文献   

川藏铁路通麦至鲁朗段地质构造对滑坡的控制作用分析     

张佳佳  王军朝  朱德明  李勇 《高校地质学报》2022,28(6):911-919

藏东南的喜马拉雅东构造结地区作为青藏高原隆升最快的地区之一,复杂的地质背景条件决定了该区工程地质问题的复杂性和特殊性,并孕育了多种地质灾害。文章通过遥感解译、无人机测绘以及野外现场调查,详细分析了喜马拉雅东构造结北西侧通麦至鲁朗段已有滑坡的发育特征,总结了地质构造对滑坡的控制作用,结果表明：（1）构造演化形成的高陡斜坡为滑坡形成提供地形条件,滑坡后缘的断裂破碎带,为雨水入渗提供通道,形成滑坡边界;（2）斜坡岩体中发育的贯通性构造节理为滑坡提供滑动条件和物质基础;（3）地震震动对岩体结构造成直接破坏,并诱发同震滑坡。多种构造作用的耦合造成了川藏铁路通麦至鲁朗段滑坡的高易发性,相关结果可为铁路修建过程的边坡灾害管控提供参考和支撑。  相似文献   

Extensional Setting of Hainan Island in Mesoproterozoic: Evidence from Granitic Intrusions in the Baoban Group     

LIU Yuheng  MAO Jingwen  QIU Kunfeng  HU Jun  WANG Lei  XU Deming 《《地质学报》英文版》2022,96(4):1199-1212

The Mesoproterozoic Baoban Group is the oldest basement in Hainan Island and has played an important role in Columbia (Nuna) supercontinent reconstructions. The Mesoproterozoic granitic intrusions in the Baoban Group are the most widely-exposed Precambrian magmatic rocks and are the key to understanding the tectonic settings of Hainan Island and its relationship with the South China Block and the Columbia supercontinent. New LA-ICP-MS zircon U-Pb dating on three mylonitic granite samples from the Tuwaishan and Baoban areas yield ages ranging from 1447 Ma to 1437 Ma, representing the absolute timing of the emplacement of the granitic intrusions. Combined with previously published geochronological data for rocks from the Baoban Group and regional mafic intrusions, it is concluded that the Baoban Group formed at 1460–1430 Ma, coeval with the emplacement of the granitic and mafic intrusions. New in-situ zircon Lu-Hf isotope analyses for the three mylonitic granite samples yielded positive εHf(t) values, ranging from +0.49 to +8.27, with model ages (TCDM) ranging from 2181 Ma to 1687 Ma, suggesting that the granitic intrusions originated from a mixed source of Paleoproterozoic crust with juvenile crust. New zircon trace element data show characteristics of high Th/U values of 0.24–1.50, steep slopes from LREE to HREE and negative Pr, Eu anomalies with positive Ce, Sm anomalies, representing typical magmatic zircons formed in continental crust. Compared with available magmatic and detrital zircon ages from Precambrian rocks in the Cathaysia Block, Yangtze Block and western Laurentia, it is inferred that Hainan Island was separated from both the Cathaysia Block and the Yangtze Block, instead being connected with western Laurentia in the Columbia supercontinent. Considering the decreasing tendency of basin deposition time along the western margin of Laurentia, it is proposed that Hainan Island was located to the north or northwest of the Belt-Purcell Supergroup, along the western margin of Laurentia, during the breakup of the Columbia supercontinent.  相似文献   

钦-杭成矿带主要金属矿床成矿系列   总被引：7，自引：0，他引：7  

徐德明  蔺志永  骆学全  张鲲  张雪辉  黄皓 《地学前缘》2015,22(2):7-24

钦-杭成矿带是华南地区最重要的Cu-Pb-Zn-Au、W-Sn-Bi-Mo和Fe-Mn-S多金属成矿带。在前人工作基础上,根据矿床的成因组合、形成构造环境及其随地质历史演化的特点,将钦-杭成矿带主要金属矿床归纳为中新元古代海底喷流沉积型铜多金属矿床、新元古代海相沉积-变质型铁锰矿床、古生代海相沉积-叠生改造型铜铅锌铁锰矿床、加里东期与花岗岩类有关的钨钼金银多金属矿床、印支期与花岗岩类有关的钨锡铌钽铀多金属矿床、燕山期与花岗岩类有关的铜铅锌金钨锡多金属矿床、与区域动力变质热液作用有关的金银矿床等7个矿床成矿系列。进而讨论了各成矿系列的主要矿床类型、矿床地质特征和时空分布规律,初步认为,中新元古代海底喷流沉积型块状硫化物铜多金属矿床与大陆边缘岛弧火山作用有关,主要分布于扬子陆块东南缘和华夏陆块西北缘古岛弧褶皱区;新元古代受变质铁锰矿床与大陆裂谷火山作用有关,并经受了后期区域变质、热变质作用的改造,主要分布于加里东期隆起区;古生代层控型铜铅锌铁锰矿床与海底热水沉积成矿作用有关,且不同程度地受到后期岩浆-热液活动的叠加改造,主要分布于海西—印支期坳陷区与隆起区的过渡部位;加里东期斑岩-夕卡岩-热液脉型钨钼金银多金属矿床与奥陶纪末—志留纪陆内造山作用有关,主要分布于加里东期隆起区;印支期斑岩-夕卡岩-热液脉型钨锡铌钽铀多金属矿床与印支板块向华南板块的俯冲碰撞有关,成矿作用发生在后碰撞伸展阶段,主要分布于海西—印支期隆起区边缘;燕山期斑岩-夕卡岩-热液脉型铜铅锌金钨锡多金属矿床与岩石圈伸展引起的玄武岩底侵作用有关,广泛分布于海西—印支期拗陷区或中生代盆地边缘;与区域动力变质热液作用有关的金银矿床成矿系列,与印支—燕山期大规模的逆冲推覆作用有关,主要发育于钦-杭结合带两侧古陆边缘。  相似文献   

Characteristics of Fengyun-4A Satellite Atmospheric Motion Vectors and Their Impacts on Data Assimilation     

Yaodeng CHEN  Jie SHEN  Shuiyong FAN  Deming MENG  Cheng WANG 《大气科学进展》2020,37(11):1222-1238

The high observation efficiency, scanning speed and observation frequency of the Fengyun-4A (FY-4A) satellite indicates the progress of Chinese geostationary meteorological satellites. The characteristics of FY-4A atmospheric motion vectors (AMVs) derived from the high-level water vapor (WV-High) channel, mid-level water vapor (WV-Mid) channel, and infrared (IR) channel of FY-4A are analyzed, and their corresponding observation errors estimated. Then, the impacts of single-channel and multi-channel FY-4A AMVs on RMAPS-ST (the Rapid-refresh Multi-scale Analysis and Prediction System—Short Term) are evaluated based on one-month data assimilation cycling and forecasting experiments. Results show that the observation errors of FY-4A AMVs from the three channels have an explicit vertical structure. Results from the cycling experiments indicate that the assimilation of AMVs from WV-High produces more apparent improvement of the wind in the upper layer, while a more positive effect in the lower layer is achieved by the assimilation of AMVs from IR. Furthermore, the assimilation of AMVs from IR is more skillful for medium and moderate precipitation than from other channels owing to the good quality of data in the lower layer in the AMVs from IR. Assimilation of FY-4A AMVs from the three channels could combine the advantages of assimilation from each individual channel to improve the wind in the upper, middle and lower layers simultaneously.  相似文献   

3.8-μm photometry during the secondary eclipse of the extrasolar planet HD 209458b     

Drake Deming †  L. Jeremy Richardson  Joseph Harrington 《Monthly notices of the Royal Astronomical Society》2007,378(1):148-152

We report infrared photometry of the extrasolar planet HD 209458b during the time of secondary eclipse (planet passing behind the star). Observations were acquired during two secondary eclipses at the NASA Infrared Telescope Facility (IRTF) in 2003 September. We used a circular variable filter (1.5 per cent bandpass) centred at 3.8 μm to isolate the predicted flux peak of the planet at this wavelength. Residual telluric absorption and instrument variations were removed by offsetting the telescope to nearby bright comparison stars at a high temporal cadence. Our results give a secondary eclipse depth of 0.0013 ± 0.0011, not yet sufficient precision to detect the eclipse, whose expected depth is  ∼0.002 –0.003  . We here elucidate the current observational limitations to this technique, and discuss the approach needed to achieve detections of hot Jupiter secondary eclipses at 3.8 μm from the ground.  相似文献