Terrestrial heat flow and lithospheric thermal structure in the Chagan Depression of the Yingen-Ejinaqi Basin,north central China     

Yinhui Zuo  Shu Jiang  Shihu Wu  Wei Xu  Jiong Zhang  Renpeng Feng  Meihua Yang  Yongshui Zhou  M. Santosh 《Basin Research》2020,32(6):1328-1346

The Chagan Depression in the Yingen-Ejinaqi Basin, located at the intersection of the Paleo-Asian Ocean and the Tethys Ocean domains is an important region to gain insights on terrestrial heat flow, lithospheric thermal structure and deep geodynamic processes. Here, we compute terrestrial heat flow values in the Chagan Depression using a large set of system steady-state temperature data from four representative wells and rock thermal conductivity. We also estimate the “thermal” lithospheric thickness, mantle heat flow, ratio of mantle heat flow to surface heat flow and Moho temperature to evaluate the regional tectonic framework and deep dynamics. The results show that the heat flow in the Chagan Depression ranges from 66.5 to 69.8 mW/m², with an average value of 68.3 ± 1.2 mW/m². The Chagan Depression is characterized by a thin “thermal” lithosphere, high mantle heat flow, and high Moho temperature, corresponding to the lithospheric thermal structure of “cold mantle and hot crust” type. We correlate the formation of the Yingen-Ejinaqi Basin to the Early Cretaceous and Cenozoic subduction of the western Pacific Plate and the Cenozoic multiple extrusions. Our results provide new insights into the thermal structure and dynamics of the lithospheric evolution in central China.  相似文献   

东南印度洋中脊澳大利亚-南极洲不整合带地区岩浆供应与构造作用沿洋脊的变化     

刘守金  林间  周志远  张帆 《海洋学报(英文版)》2020,39(1):118-129

We analyzed seafloor morphology and geophysical anomalies of the Southeast Indian Ridge(SEIR) to reveal the remarkable changes in magma supply along this intermediate fast-spreading ridge. We found systematic differences of the Australian-Antarctic Discordance(AAD) from adjacent ridge segments with the residual mantle Bouguer gravity anomaly(RMBA) being more positive, seafloor being deeper, morphology being more chaotic, M factors being smaller at the AAD. These systematic anomalies, as well as the observed Na_(8.0) being greater and Fe_(8.0) being smaller at AAD, suggest relatively starved magma supply and relatively thin crust within the AAD.Comparing to the adjacent ridges segments, the calculated average map-view M factors are relatively small for the AAD, where several Oceanic Core Complexes(OCCs) develop. Close to 30 OCCs were found to be distributed asymmetrically along the SEIR with 60% of OCCs at the northern flank. The OCCs are concentrated mainly in Segments B3 and B4 within the AAD at ～124°–126°E, as well as at the eastern end of Zone C at ～115°E. The relatively small map-view M factors within the AAD indicate stronger tectonism than the adjacent SEIR segments.The interaction between the westward migrating Pacific mantle and the relatively cold mantle beneath the AAD may have caused a reduction in magma supply, leading to the development of abundant OCCs.  相似文献   

辽东中生代晚期和古近纪玄武岩及深源捕虏晶--对岩石圈地幔性质的制约   总被引：8，自引：0，他引：8  

王微  许文良  纪伟强  杨德彬  裴福萍 《高校地质学报》2006,12(1):30-40

辽东地区玄武岩的K-Ar定年结果表明,曲家屯玄武岩形成于晚白垩世,K-Ar年龄为81．58±2．46Ma;乱石山子玄武岩形成于古近纪,K-Ar年龄为58．36±1．64Ma。本区玄武岩含有丰富的橄榄石、单斜辉石和角闪石捕虏晶。乱石山子玄武岩中橄榄石捕虏晶的Mg^#值（79．5-88．5之间,平均值为84）较曲家屯玄武岩中橄榄石捕虏晶Mg^#值（77．0～79．8之间,平均值为78．4）偏高;单斜辉石捕虏晶为透辉石,其从核部到边部的Mg^#等变化趋势与橄榄石类似;斜方辉石捕虏晶为占铜辉石,其Mg^#值介于85．2-87．6之间,平均值为86．4。捕虏晶发育的环状裂隙、扭折带、矿物成分环带以及捕虏晶与主岩Mg^#值之间的不平衡均暗示它们为玄武质岩浆上升捕获的早期岩浆晶出矿物的堆晶体。玄武岩的岩石地球化学分析结果表明：（1）它们属于碱性系列,为碱性玄武岩,曲家屯玄武岩较乱石山子玄武岩贫硅、镁,富钙、铝,它们均具有原始岩浆的特征;（2）二者具有相似的稀土元素配分模式,但曲家屯玄武岩轻稀土元素总量更高,且轻重稀土元素分离程度高;（3）二者具有相似的Sr-Nd同位素组成,Isr和εNd（t）值分别介于0．7039～0．7045和＋1．60～＋3．69,反映了亏损的岩石圈地幔特征。  相似文献   

印度板块岩石圈地幔向北俯冲到羌塘地体之下的远震P波层析成像证据   总被引：7，自引：3，他引：4       下载免费PDF全文

郑洪伟  李廷栋  高锐  赵大鹏  贺日政 《地球物理学报》2007,50(5):1418-1426

利用PASSCAL、INDEPTH Ⅱ、INDEPTH Ⅲ、HIMNT等研究计划,及中国新疆地学断面和国家973项目在青藏高原布设的流动台站记录的到时数据,以及自1990年1月到2004年2月全球地震事件的震相报告,作者对覆盖印度大陆的恒河平原和整个青藏高原的305个地震台站记录的9649个远震事件,共139021条P波初至到时资料进行了层析成像反演．结果表明：印度岩石圈地幔在不同的位置向北俯冲的形态不同,但俯冲前缘都到达羌塘地体之下．沿88°E剖面显示,厚约100 km的印度岩石圈地幔从南部的恒河平原向北一直俯冲到青藏高原之下．在主边界逆冲断裂之下100 km深度处以约22°角度开始向北俯冲,俯冲最前缘到达羌塘地体的中部地区约34°N,之后进入上地幔深处．而沿北东方向的剖面则显示,印度岩石圈地幔以近水平的角度俯冲到青藏高原之下,向北越过班公－怒江缝合带,到达33°N附近,然后以大角度近乎垂直地向下俯冲断离,并引起地幔热物质的上涌,形成羌塘地体之下大规模的低速带．  相似文献   

大陆岩石圈研究进展   总被引：5，自引：0，他引：5  

陈凌  朱日祥  王涛 《地学前缘》2007,14(2):58-75

从地震学、地球化学、岩石学等不同学科的角度,对大陆岩石圈研究进展做了简要介绍。不同学科的最新研究成果表明,岩石圈在热状态、化学成分和力学行为等方面具有高度非均匀性。这不仅表现为岩石圈性质和结构随深度的变化,而且还反映在不同时代、大陆与海洋以及克拉通和造山带岩石圈结构特征的显著差异上。性质和结构的差异体现了岩石圈形成和长期演化过程的复杂性。我们认为,不同岩石圈块体之间、岩石圈与深部对流地幔之间普遍存在着相互作用。这种相互作用被认为是稳定克拉通岩石圈遭受改造甚至破坏的深部机制,同时还是地球深、浅部物质交换的重要方式,因而显著影响着地球深部的对流和地表的构造过程。值得注意的是,由于岩石圈本身定义的模糊性及其厚度的不确定性,地震活动与岩石圈强度之间的关系以及大陆岩石圈演化的规律性等问题仍有待于进一步的研究和探索。  相似文献   

克拉通岩石圈地幔的形成与破坏:大洋板块俯冲的贡献     

汤艳杰 《地球科学与环境学报》2021,(2):237-243

克拉通是地球上最古老的大陆地块.克拉通之所以能够长期稳定存在,主要是因为它具有巨厚、刚性的岩石圈地幔.古老克拉通岩石圈地幔具有高度难熔(富Mg、贫Fe)的特点,其密度较下伏软流圈小,能够"漂浮"在软流圈之上而长期存在.古老克拉通岩石圈地幔是在地球早期壳幔分异之后形成的,其形成可能与大洋板块的俯冲作用密切相关.典型的克拉...  相似文献   

Early Cretaceous Metasomatized Lithospheric Mantle beneath the Central Jiangnan Orogen in South China: Geochemical and Sr-Nd Isotope Evidence from the Tuanshanbei Dolerite     

WANG Cheng  WEI Hantao  LIU Qingquan  YANG Zhao 《《地质学报》英文版》2024,98(3):602-616

It is well established that Cretaceous magmatism in the South China Block (SCB) is related to the Paleo-Pacific subduction. However, the starting time and the associated deep crust-mantle processes are still debatable. Mafic dike swarms carry important information on the deep earth (including mantle) geodynamics and geochemical evolution. In the Jiangnan Orogen (South China), there is no information on whether the Mesozoic magmatic activities in this region are also directly related to the Pacific subduction or not. In this study, we present detailed zircon U-Pb geochronological, whole-rock element and Sr-Nd isotope data for Early Cretaceous Tuanshanbei dolerite dikes, and provide new constraints on the condition of the lithospheric mantle and mantle dynamics of the SCB during that time. LA-ICP-MS zircon U-Pb dating suggests that this dolerite erupted in the Early Cretaceous (~145 Ma). All samples have alkaline geochemical affinities with K2O + Na2O = 3.11–4.04 wt%, K2O/Na2O = 0.50–0.72, and Mg# = 62.24–65.13. They are enriched in LILE but depleted in HFSE with higher initial 87Sr/86Sr ratio (0.706896–0.714743) and lower εNd(t) (?2.61 to ?1.67). They have high Nb/U, Nb/La, La/Sm and Rb/Sr, and low La/Nb, La/Ta, Ce/Pb, Ba/Rb, Tb/Yb and Gd/Yb ratios. Such geochemical signatures suggest that the fractional crystallization is obvious but crustal contamination play a negligible role during magmatic evolution. Tuanshanbei dolerite were most likely derived from low-degree (2%–5%) partial melting of a phlogopite-bearing mantle material consisted of ~85% spinel peridotite and ~15% garnet peridotite previously metasomatized by asthenosphere-derived fluids/melts with minor subduction-derived fluids/melts. Slab-rollback generally lead to the upwelling of the hot asthenosphere. The upwelling of asthenosphere consuming the lithospheric mantle by thermo-mechanical-chemical erosion. The lithospheric mantle may have partially melted due to the heating by the upwelling asthenosphere and lithospheric extension. It is inferred that the Tuanshanbei dolerite might be associated with the initial slab rollback and corresponding lithospheric extension occurred potentially at ca. 145 Ma.  相似文献   

302铀矿床方解石C-O同位素组成与成矿动力学背景研究   总被引：8，自引：0，他引：8  

张国全  胡瑞忠  商朋强  田建吉  双燕 《矿物学报》2008,28(4)

302铀矿床规模大,垂幅深(达1000多米),是我国华南主要产铀花岗岩型铀矿床之一。研究表明该矿床的方解石是经大气降水与围岩发生水岩反应后的流体去气沉淀的;矿化剂∑CO2主要源自受控于岩石圈伸展导致的地幔去气,对铀成矿的作用一方面表现为加入到贫矿化剂的地下水中以便铀元素迁移,另一方面表现在从成矿流体中逸出,改变热液络离子组成,导致铀沉淀成矿;印支碰撞运动使华南地壳叠加增厚,部分熔融含铀结晶基底,为产铀岩体提供丰富的成矿物质来源;白垩纪-古近纪地壳拉张、岩石圈伸展所形成的深大断裂等不仅是矿化剂∑CO2主要通道,而且还是控制铀矿床形成的关键因素。  相似文献   

New limits on the motion between India and Australia since chron 5 (11 Ma) and implications for lithospheric deformation in the equatorial Indian Ocean   总被引：1，自引：0，他引：1  

Jean-Yves Royer  Richard G. Gordon  Charles DeMets  Peter R. Vogt 《Geophysical Journal International》1997,129(1):41-74

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Modern tectonic regime in the Tyrrhenian area: observations and models     

Gianna Bassi  Roberto Sabadini  Samira Rebaï 《Geophysical Journal International》1997,129(2):330-346

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