岩浆底侵的热-流变学效应及对峨眉山大火成岩省的启示   总被引：1，自引：1，他引：0  

王振华  陈赟  陈林  宋海斌 《岩石学报》2018,34(1):91-102

岩浆底侵在大陆地壳的形成和演化过程中起着非常重要的作用。本文基于二维热传导方程模拟不同规模的地壳底侵产生的热-流变学效应,以及幔源岩浆温度和含水量对底侵厚度的影响;并以现有的岩石地球化学分析、深部地球物理探测结果为约束,模拟了峨眉山大火成岩省内带幔源岩浆底侵对应的地表热流随时间演化,探讨了形成幔源岩浆底侵的潜温和初始熔融的深度制约。结果显示:1)幔源岩浆底侵引起的热扰动的耗散时间取决于岩浆底侵的初始厚度。以幔源岩浆侵入温度为1300℃,20km厚的地壳底侵为例,热扰动完全耗散需经历约150Myr;而5km厚的地壳底侵,只需经历50Myr热扰动已基本耗散殆尽。2)在初始阶段,岩浆底侵会造成岩石圈强度的显著降低;随着热耗散的进行,岩石圈强度会逐渐恢复;在热扰动耗散殆尽之后,岩石圈强度反倒比底侵前的岩石圈强度更大。这表明岩浆底侵不但可以导致地壳增厚,还会最终导致岩石圈的强化。3)温度对地壳底侵厚度的影响比含水量的影响要大得多。将我们的模型应用于峨眉山大火成岩省,结果表明内带地壳底侵的热耗散需持续上百个百万年,岩浆潜温超过1500℃,初始熔融深度超过200km。  相似文献   

江西印支期蔡江岩体中暗色微粒包体的发现及其地质意义     

刘运超  姜耀辉  青龙  杜佛光 《高校地质学报》2022,28(4):473-483

文章报道了江西蔡江花岗质岩体中发现暗色微粒包体,以及这些包体的地质、岩相学、LA-ICP-MS锆石U-Pb年代学和元素地球化学特征。包体多呈椭圆状,显示淬冷边和反向脉,具有典型的岩浆结构并含有针状磷灰石,有的包体含有长石捕虏晶。包体具有相对较低的SiO₂（低至57.05 wt%）和较高的MgO+Fe₂O₃（高达14.21 wt%）含量。LA-ICP-MS锆石U-Pb定年数据表明,包体形成于晚三叠世（224 Ma）,与寄主花岗岩（230~228 Ma）在误差范围内基本一致。上述特征表明,包体是离散的幔源偏基性岩浆团或者是幔源与寄主岩浆混合的产物。原始包体岩浆属于超钾质岩浆,可能是通过岩石圈地幔中交代成因的金云母辉石岩脉发生部分熔融而形成的。暗色微粒包体的发现为幔源岩浆底侵提供了直接证据,从而为蔡江花岗质岩石形成于较高温度提供佐证。该研究对于进一步探讨华南印支期花岗岩形成的热源机制具有意义。  相似文献   

华北克拉通北缘显生宙四次底侵作用及其构造-岩浆活动与深部背景     

邵济安  周新华  张履桥 《地学前缘》2020,27(4):124-134

通过对华北克拉通北缘显生宙四次(P₁,T₃,J₁,K₁)底侵作用的研究,将华北克拉通的活化与岩石圈深部地幔物质的底辟体上涌联系起来。不同阶段底侵作用在岩浆来源深度、与构造格局关系、对地壳垂向增生的贡献、幔源物质脉动式上涌等方面的差异与变化,显示它们是一个分阶段连续热演化的深部过程,其动力学机制是深部的高热流和地幔物质的向上运移。对应于地幔物质上涌,必然存在同期的地幔底辟体隆起的岩石圈结构变化。通过对华北中生代盆山系形成机制的讨论,认为该区高分辨率面波层析成像所显示的地幔底辟体上涌的特征可以反映中生代岩石圈底侵作用的深部背景。  相似文献   

Lower crustal melting via magma underplating: Elemental and Sr–Nd–Pb isotopic constraints from late Mesozoic intermediate–felsic volcanic rocks in the northeastern North China Block     

CHAOWEN LI  FENG GUO  WEIMING FAN 《Island Arc》2011,20(4):477-499

Ar–Ar dating, major and trace element analyses, and Sr–Nd–Pb isotope results of two groups of Lower Cretaceous (erupted at 126 and 119 Ma, respectively) intermediate–felsic lava from the northeastern North China Block (NCB) suggest their derivation from melting of mixtures between the heterogeneous lower crust and underplated basalts. Both groups exhibit high‐K calc‐alkaline to shoshonitic affinities, characterized by light rare earth element (LREE) and large ion lithophile element (LILE) enrichment and variable high field strength element (HFSE, e.g. Nb, Ta and Ti) depletion, and moderately radiogenic Sr and unradiogenic Nd and Pb isotopic compositions. Compared with Group 2, Group 1 rocks have relatively higher K₂O and Al₂O₃/(CaO + K₂O + Na₂O) in molar ratio, higher HFSE concentrations and lower Nb/Ta ratios, and higher Sr–Nd–Pb isotope ratios. Group 1 rocks were derived from a mixture of an enriched mantle‐derived magma and a lower crust that has developed radiogenic Sr and unradiogenic Nd and Pb isotopic compositions, whereas the Group 2 magmas were melts of another mixture between the same mantle‐derived component and another type of lower crust having even lower Sr, Nd, and Pb isotopic ratios. Shift in source region from Group 1 to Group 2 coincided with a change in melting conditions: hydrous melting of both the underplated basalt and the lower crust produced the earlier high‐Nb and low‐Nb/Ta melts with little or no residual Ti‐rich phases; while the younger low‐Nb and high‐Nb/Ta magmas were melted under a water‐deficient system, in which Ti‐rich phases were retained in the source. Generation of the two groups of intermediate–felsic volcanic rocks was genetically linked with the contemporaneous magma underplating event as a result of lithospheric thinning in the eastern NCB.  相似文献   

Deep crustal structure and rheology of the Gascoyne volcanic margin,western Australia     

Frey  Øivind  Planke  Sverre  Symonds  Phillip A.  Heeremans  Michel 《Marine Geophysical Researches》1998,20(4):293-311

Interpretation of deep seismic reflection data across the Gascoyne Margin reveals six distinct seismic facies units related to the tectono-magmatic breakup history. On the outer Exmouth Plateau four large scale units are identified: (1) an extensively block-faulted upper crust; (2) a middle-crustal unit of discontinuous, undulatory reflectors; (3) a reflection-free deep crustal unit; and (4) a lower-crustal band of low-frequency, high-amplitude reflectors. Two additional units are found near the continent-ocean boundary (COB); (5) seaward-dipping reflectors (SDR); and (6) landward-dipping reflectors in the lower crust below the SDR. The lower-crustal high-reflectivity band, located near the top of a high-velocity unit (V_p > 7 kms^–1), is interpreted as magmatic underplating. There is a spatial correlation between the underplated area and the presence of extensive upper-crustal block-faulting and intrusive rocks in the shallow crust. The undulatory middle-crustal reflector unit is also only identified in the outer plateau area, and is interpreted as a zone in which the upper-crustal faults terminate. The inner parts of the margin consist of a deep basin showing little upper-crustal faulting and no evidence of middle crustal deformation or underplating. Theoretical modeling of the effect of rifting and magmatic underplating on crustal strength profiles suggests that the brittle-ductile transition may migrate at least 5 km upwards during several million years after the underplating event. Based on the seismic interpretation and crustal strength modeling we propose that the seismic structure of the outer Exmouth Plateau is severely modified by a transient change in the crustal rheological structure associated with magmatic underplating.  相似文献   

从地壳上地幔构造看大陆碰撞带岩石圈的克拉通化   总被引：1，自引：0，他引：1  

杨文采  于常青 《地质论评》2014,60(4):721-740

本篇讨论超级大陆汇聚后逐渐变为克拉通或扩大克拉通的作用过程,即指经及大陆碰撞地体汇聚后新形成的大陆块逐渐转变为刚性克拉通的作用过程。增生大陆岩石圈的克拉通化的作用后果,包括大陆地壳密度的增加,岩石圈地幔的增厚和大地热流值的下降,使大陆岩石圈逐渐刚性强化。大陆碰撞后形成的大陆块必须经过克拉通化的过程,才能逐渐成为刚性克拉通。作用过程主要包括:①上地壳沉积碎屑岩石结晶岩化和中地壳岩石角闪岩化;②下地壳岩石基性化;③大陆碰撞带下凹莫霍面的磨平;④岩石圈地幔底侵加厚形成陆根。从大陆碰撞带转变为克拉通的过程也是岩石圈地幔不断增厚而地壳缓慢变硬变冷的过程。这个过程包含以下作用:区域变质作用,交代作用和岩石圈幔源岩浆的底侵。这个过程时间尺度比碰撞造山作用大一个级次。长期的底侵作用使地壳岩石密度和强度不断加大,改变岩层的矿物成分和局部结构。当大陆岩石圈克拉通化到一定程度之后,由于下方软流圈的热能供应逐渐减缓,使岩石圈地温梯度缓慢下降,最终结果会形成大陆根。由于显生宙大陆碰撞带岩石圈强度弱,大陆碰撞时更容易造成岩石圈变形,因此大陆碰撞的板内效应主要发生在大陆内的显生宙碰撞带。显生宙大陆碰撞带如果再次受到大陆碰撞板内效应的作用,其克拉通化的过程必然会推迟。  相似文献   

Crustal accretion beneath the Koyna coastal region (India) and Late Cretaceous geodynamics     

A.P Singh  D.M Mall   《Tectonophysics》1998,290(3-4):285-297

In 1967 a major earthquake in the Koyna region attracted attention to the hitherto considered stable Indian shield. The region is covered by a thick pile of Deccan lava flows and characterized by several hidden tectonic features and complex geophysical signatures. Although deep seismic sounding studies have provided vital information regarding the crustal structure of the Koyna region, much remains unknown. The two available DSS profiles in the region have been combined along the trend of Bouguer gravity anomalies. Unified 2-D density modelling of the Koyna crust/mantle suggests a ca. 3 km thick and 40 km wide high velocity/high density anomalous layer at the base of the crust along the coastline. The thickness of this anomalous layer decreases gradually towards the east and ahead of the Koyna gravity low the layer ceases to be visible. Based on the seismic and gravity data interpretation in the geodynamical/rheological boundary conditions the anomalous layer is attributed to igneous crustal accretion at the base of the crust. It is suggested that the underplated layer is the imprint of the magmatism caused by the deep mantle plume when the northward migrating Indian plate passed over the Reunion hotspot.  相似文献   

南海东北部下地壳高速层的成因探讨   总被引：2，自引：0，他引：2  

刘安  武国忠  吴世敏 《地质论评》2008,54(5):609-616

通过对南海北部大陆边缘地壳结构分析,指出南海东北部存在下地壳高速层,大致分布在112°E~120°E,19°N~22°N的陆坡和拉张程度大的陆架地区,呈NEE向延伸,在海底地震仪剖面上最大的厚度有8km,向南海海盆方向减薄。通过对比综合分析认为,高速层物质组成是底侵作用形成的熔岩垫,由于伸展作用,南海海底扩张（30Ma）前后底侵作用形成了熔岩垫,并促使南海北部大陆边缘地壳抬升,导致区域性抬升剥蚀。  相似文献   

关于底侵作用和拆沉作用在南海中的指示意义   总被引：2，自引：0，他引：2  

蔡周荣  夏斌  王冉  吕宝凤 《海洋通报》2007,26(6):48-52

南海位于印度板块、欧亚板块和太平洋板块之间,是世界上最大的边缘海。许多学者对其成因模式和动力学机制进行过多方面的探讨,但往往只注重地壳浅部和侧向碰撞的研究,而忽视了深部的壳幔相互作用。从地形地貌、岩石地球化学、地球物理学、岩相古地理学等地质事实出发,论述了南海存在着大规模的底侵作用和拆沉作用,并在前人研究的基础上,建立了简单的以底侵作用和拆沉作用为主的壳幔相互作用模型来模拟南海的形成演化过程,指出底侵作用和拆沉作用是南海形成演化过程中深部的主要推动力,对南海的形成演化有着非常重要的影响。  相似文献   

Crustal growth in south-eastern Australia—evidence from lower crustal eclogitic and granulitic xenoliths     

SUZANNE Y. WASS  J. D. HOLLIS 《Journal of Metamorphic Geology》1983,1(1):25-45

Mafic and ultramafic xenoliths in a basaltic cone at The Anakies in south-eastern Australia are geochemically equivalent to continental basaltic magmas and cumulates. The xenolith microstructures range from recognizably meta-igneous for intrusive rocks to granoblastic for garnet pyroxenites. Contact relationships between different rock types within some xenoliths suggest a complex petrogenesis of multiple intrusive, metamorphic and metasomatic events at the crust/mantle boundary during the evolution of south-eastern Australia. Unaltered spinel lher-zolite, typical of the uppermost eastern Australian mantle, is interleaved with or veined by the metamorphosed intrusive rocks of basaltic composition. Geothermobarometry calculations by a variety of methods show a concordance of equilibration temperatures ranging from 880°C to 980°C and pressures of 12 to 18 kbar (1200-1800 mPa). These physical conditions span the gabbro to granulite to eclogite transition boundaries. The water-vapour pressure during equilibration is estimated to be about 0.5% of the load pressure, using amphibole breakdown data. Large fluid inclusions of pure CO₂ are abundant in the mineral phases in the xenoliths, and it is suggested that flux of CO₂ from the mantle has been an important heat source and fluid medium during metamorphism of the mafic and ultramafic protoliths at the lower crust/upper mantle boundary. The calculated pressures and temperatures suggest that the south-eastern Australian crust has sustained a high geothermal gradient. In addition, the nature of the mineral assemblages and the contact relationships of granulitic rock with spinel lherzolite, characteristic of mantle material, suggest that the Moho is not a discrete feature in this region, but is represented by a transition zone approximately 20 km thick. These inferences are in agreement with geophysical data (including seismic, heat-flow and electrical resistivity data) determined for south-eastern Australia. Underplating at the crust/mantle boundary by continental basaltic magmas may be an important alternative or additional mechanism to the conventional andesite model for crustal accretion.  相似文献