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21.
Geochemical data are presented for the meta-igneous, mafic-ultramafic complex near Finero. This complex is in contact with a phlogopite-bearing mantle peridotite and is subdivided into the Internal Gabbro unit, the Amphibole Peridotite unit, and the External Gabbro unit. The Internal Gabbro and the Amphibole Peridotite units consist of coarse-grained, chemically heterogeneous cumulates, whereas the External Gabbro unit is generally massive, chemically more uniform and approximately representative of the residual melt with MgO contents between 6.6 and 9.1% and Mg numbers between 38 and 58. Both whole-rock and mineral contents of Ni and Cr are significantly higher (at similar Mg numbers) in the Amphibole Peridotite unit than in the Internal Gabbro unit. The most straightforward interpretation of this is that the Amphibole Peridotite unit accumulated after the influx of fresh mafic (or ultramafic) magma into the magma chamber. Major-element chemical trends are continuous from the Amphibole Peridotite unit to the External Gabbro unit and are consistent with closed-system fractionation with no further addition of magma or contamination by wall or roof rock assimilation. In the External Gabbro unit, total FeO and TiO2 contents are strongly correlated with each other (and with P2O5 and Zr) and reach values as high as 19 and 4%, respectively, indicating an advanced degree of crystal fractionation along a tholeftic trend. The External Gabbro samples have generally smooth normalized trace element patterns, which are consistent with being representative of a liquid composition. The residual nature of the External Gabbro magma is also indicated by negative Eu and Sr anomalies, clear evidence for prior feldspar fractionation. REE patterns are otherwise indistinguishable from N-type MORB, but Th and U are significantly more depleted than in MORB. This Th and U depletion is similar to that found in olivine basalts and picrites on Iceland and Hawaii; its origin is not well understood. No evidence is seen for any assimilation of crystal material, in sharp contrast with the situation of the igneous complex in Val Sesia near Balmuccia, where the magma composition is dominated by assimilation of crust. We suggest that the heat provided by at most two injections of magma near Finero was insufficient to induce crystal anatexis, in contrast with the excess heat supplied by multiple magma injections at Balmuccia.  相似文献   
22.
τ-P域地震资料三维叠前深度偏移及其实用算法   总被引:3,自引:2,他引:3       下载免费PDF全文
本文提出了在τ-P域实现三维叠前深度偏移的计算方法,该方法把地震道集由时-空域变换到τ-P域,然后对共P数据体进行相移或相移加插值偏移,将偏移后的各共P数据体叠加得到叠前深度偏移结果.该算法能够实现陡倾地层的正确归位,降低偏移处理维数,减少计算机内存需求,易于并行处理,但是计算量和所花费的计算机时间仍然很大.为此我们又提出了针对目的层的分时(层)偏移方法,由于只考虑目的层,可节省大量的计算时间.文中以二维实际地震资料及三维数值模型资料的处理说明了上述方法的可行性与有效性.  相似文献   
23.
青藏高原南羌塘基性岩墙群U-Pb和Sm-Nd同位素定年及构造意义   总被引:17,自引:0,他引:17  
羌塘地区是青藏高原古特提斯研究的关键地区,羌塘南部地区基性岩墙群的侵位时代与构造背景对确定古特提斯阶段联合古陆解体的具体时间和青藏高原构造演化有重要意义。选择单颗粒锆石U-Pb法和全岩Sm-Nd等时线法对基性岩墙进行定年研究,获得了(312±4)Ma单颗锆石U—Pb谐合线年龄和(299±13)Ma和(314±5)Ma两个Sm-Nd全岩等时年龄。结合区域地质资料研究认为,基性岩墙群为羌塘地块裂离作用的产物,所获得的同位素年龄代表了基性岩墙群的侵位时间,为羌塘地块裂解提供了构造事件年龄,为重塑龙木错—双湖古特提斯洋盆的形成演化过程提供了重要信息。  相似文献   
24.
西准噶尔紫苏花岗岩成因岩石学研究   总被引:8,自引:1,他引:8  
紫苏花岗岩呈岩体形式侵入于石炭纪地层中.又为碱长花岗岩侵入.紫苏花岗岩由斜方辉石、单斜辉石、铁橄榄石、条纹长石、石英组成.以正εNd为特征(εNd= 4.8- 5.8)矿物组成、结构和野外产状表明:这些紫苏花岗岩是火成成因的.温压计算估测其结晶条件是T=700~800℃,P=420~575kPa.紫苏花岗岩中有小的富云母包体和巨大的条带状捕虏体.前被认为是残留体,后与其围岩.火山碎屑岩相当.残留体中较低的εNd正值(εNd= 2.6- 3.5)要求新生的下部地壳是紫苏花岗岩的主要源岩:来自这些源岩的紫苏花岗岩的母岩浆在结晶前与一些来自于亏损地幔中的融体混合.该地区体积巨大的碱性花岗岩可能也来自相同的岩浆源,只不过它是在较浅的地壳深度上结晶的.  相似文献   
25.
传统型铂族矿产,系指与镁铁质岩浆成矿作用有关的铂族矿产资源。华力西运动时期,扬子地台西南缘沿超壳深断裂带发生的大陆裂谷作用,为来自上地幔的镁铁质(拉斑玄武岩质)岩浆的上涌和侵位提供了极为有利的前提条件。含铂基性超基性岩的时空分布,受到大陆裂谷作用的主要发生发展时期和裂谷活动带的控制。通过对典型矿床特征及其成矿作用的探讨,论述了扬子地台西南缘主要的铂族矿床类型;并从四维成矿的角度,阐述了对区域成矿规律的一些基本认识。  相似文献   
26.
The Vinalhaven intrusive complex consists mainly of coarse-grainedgranite, inward-dipping gabbro–diorite sheets, and a fine-grainedgranite core. Small bodies of porphyry occur throughout thecoarse-grained granite. The largest porphyry body (roughly 0·5km by 2·5 km) occurs with coeval gabbro, hybrid rocks,and minor fine-grained granite in the Vinal Cove complex, whichformed during the waning stages of solidification of the coarse-grainedVinalhaven granite. Porphyry contacts with surrounding coarse-grainedgranite are irregular and gradational. Compositions of wholerocks and minerals in the porphyry and the coarse-grained graniteare nearly identical. Neighboring phenocrysts in the porphyryvary greatly in degree of corrosion and reaction, indicatingthat the porphyry was well stirred. Thermal rejuvenation ofa silicic crystal mush by a basaltic influx can explain thecomposition and texture of the porphyry. Comparable rejuvenationevents have been recognized in recent studies of erupted rocks.Weakly corroded biotite phenocrysts in the porphyry requirethat hydrous interstitial melt existed in the granite duringremelting. Field relations, along with thermal calculations,suggest that cooling and crystallization of coeval mafic magmacould have generated the porphyry by thermal rejuvenation ofgranite crystal-mush containing about 20% melt. Field relationsalso suggest that some of the porphyry matrix may representnew felsic magma that was emplaced during remelting. KEY WORDS: granite; magma chamber; mafic replenishment; rejuvenation  相似文献   
27.
The structural organization of a giant mafic dyke swarm, the Okavango complex, in the northern Karoo Large Igneous Province (LIP) of NE Botswana is detailed. This N110°E-oriented dyke swarm extends for 1500 km with a maximum width of 100 km through Archaean basement terranes and Permo-Jurassic sedimentary sequences. The cornerstone of the study is the quantitative analysis of N>170 (exposed) and N>420 (detected by ground magnetics) dykes evidenced on a ca. 80-km-long section lying in crystalline host-rocks, at high-angle to the densest zone of the swarm (Shashe area). Individual dykes are generally sub-vertical and parallel to the entire swarm. Statistical analysis of width data indicates anomalous dyke frequency (few data <5.0 m) and mean dyke thickness (high value of 17 m) with respect to values classically obtained from other giant swarms. Variations of mean dyke thicknesses from 17 (N110°E swarm) to 27 m (adjoining and coeval N70°E giant swarm) are assigned to the conditions hosting fracture networks dilated as either shear or pure extensional structures, respectively, in response to an inferred NNW–SSE extension. Both fracture patterns are regarded as inherited brittle basement fabrics associated with a previous (Proterozoic) dyking event. The Okavango N110°E dyke swarm is thus a polyphase intrusive system in which total dilation caused by Karoo dykes (estimated frequency of 87%) is 12.2% (6315 m of cumulative dyke width) throughout the 52-km-long projected Shashe section. Assuming that Karoo mafic dyke swarms in NE Botswana follow inherited Proterozoic fractures, as similarly applied for most of the nearly synchronous giant dyke complexes converging towards the Nuanetsi area, leads us to consider that the resulting triple junction-like dyke/fracture pattern is not a definitive proof for a deep mantle plume in the Karoo LIP.  相似文献   
28.
Abstract  Abundant mafic microgranular enclaves (MMEs) extensively distribute in granitoids in the Gangdisê giant magmatic belt, within which the Qüxü batholith is the most typical MME‐bearing pluton. Systematic sampling for granodioritic host rock, mafic microgranular enclaves and gabbro nearby at two locations in the Qüxü batholith, and subsequent zircon SHRIMP II U‐Pb dating have been conducted. Two sets of isotopic ages for granodioritic host rock, mafic microgranular enclaves and gabbro are 50.4±1.3 Ma, 51.2±1.1 Ma, 47.0±1 Ma and 49.3±1.7 Ma, 48.9±1.1 Ma, 49.9±1.7 Ma, respectively. It thus rules out the possibilities of mafic microgranular enclaves being refractory residues after partial melting of magma source region, or being xenoliths of country rocks or later intrusions. Therefore, it is believed that the three types of rocks mentioned above likely formed in the same magmatic event, i.e., they formed by magma mixing in the Eocene (c. 50 Ma). Compositionally, granitoid host rocks incline towards acidic end member involved in magma mixing, gabbros are akin to basic end member and mafic microgranular enclaves are the incompletely mixed basic magma clots trapped in acidic magma. The isotopic dating also suggested that huge‐scale magma mixing in the Gangdisê belt took place 15–20 million years after the initiation of the India‐Asia continental collision, genetically related to the underplating of subduction‐collision‐induced basic magma at the base of the continental crust. Underplating and magma mixing were likely the main process of mass‐energy exchange between the mantle and the crust during the continental collision, and greatly contributed to the accretion of the continental crust, the evolution of the lithosphere and related mineralization beneath the portion of the Tibetan Plateau to the north of the collision zone.  相似文献   
29.
30.
郭晶  李云帅  张建新 《地质学报》2020,94(9):2698-2711
大陆碰撞造山带中高压麻粒岩的 P- T- t 轨迹研究对于理解造山带的热演化历史及大陆地壳的形成与演化具有重要的意义,然而,如何连接同位素年龄与变质演化过程是恢复和建立 P- T- t 轨迹的重点和难点。本文通过对南阿尔金巴什瓦克地区基性麻粒岩的详细岩相学研究,认为该基性麻粒岩经历了原岩阶段(M1)、峰期变质阶段(M2)、峰后退变质阶段(M3)以及晚期角闪岩相- 绿片岩相退变质阶段(M4)。其中,传统矿物温压计和矿物微量元素温压计获得该基性麻粒岩所记录的峰期变质条件分别为17. 5~22. 6 kbar,901~985℃ 和17~28 kbar,1012~1049℃,退变质阶段的温压条件为7. 6~10. 7 kbar,750~810℃。此外,锆石U- Pb 年代学结果表明基性麻粒岩的变质时代为491±3. 5 Ma (MSWD=0. 62),结合锆石和石榴子石的微量元素分配系数以及前人的实验岩石学数据,认为该变质时代记录了早古生代高压- 超高温的变质事件,进而恢复了南阿尔金基性麻粒岩所记录的顺时针 P- T- t 轨迹。  相似文献   
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