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Many Neo-Tethyan ophiolitic bodies are well exposed as thrust-slices in Central Anatolia and are predominantly represented by massive hornblende gabbros, most of which are cut by Supra Subduction Zone (SSZ) plagiogranites. The allochthonous gabbros are distinct from their autochthonous counterparts, with their mineralogy including both igneous hornblende, relict diopside rimmed by replacement hornblende and their chemical composition corresponding mostly to gabbro rather than diorite.The results of major and trace element analyses of forty-two samples, and REE analyses of nine samples, indicate that the hornblende gabbros are SSZ-type and formed from a wet magma by high-degree partial melting of peridotite possibly coupled with contamination by predominantly neighbouring-slab derived fluids within an intra-oceanic back-arc basin. The mafic magmas then underwent high-level fractional crystallization involving titaniferous magnetite, diopside, tschermakite and possibly olivine. Emplacement was followed by extensive ocean–floor metamorphism, which has induced crystallization (or recrystallization) of chlorite, biotite, amphiboles and mobilisation of most of the major elements such as alkali and alkali earth elements, and some LREE. 相似文献
3.
《Journal of Asian Earth Sciences》2006,26(6):883-891
Many Neo-Tethyan ophiolitic bodies are well exposed as thrust-slices in Central Anatolia and are predominantly represented by massive hornblende gabbros, most of which are cut by Supra Subduction Zone (SSZ) plagiogranites. The allochthonous gabbros are distinct from their autochthonous counterparts, with their mineralogy including both igneous hornblende, relict diopside rimmed by replacement hornblende and their chemical composition corresponding mostly to gabbro rather than diorite.The results of major and trace element analyses of forty-two samples, and REE analyses of nine samples, indicate that the hornblende gabbros are SSZ-type and formed from a wet magma by high-degree partial melting of peridotite possibly coupled with contamination by predominantly neighbouring-slab derived fluids within an intra-oceanic back-arc basin. The mafic magmas then underwent high-level fractional crystallization involving titaniferous magnetite, diopside, tschermakite and possibly olivine. Emplacement was followed by extensive ocean–floor metamorphism, which has induced crystallization (or recrystallization) of chlorite, biotite, amphiboles and mobilisation of most of the major elements such as alkali and alkali earth elements, and some LREE. 相似文献
4.
The origin of the Cretaceous gabbros in the Fujian coastal region of SE China: implications for deformation-accompanied magmatism 总被引：2，自引：0，他引：2
Zhihong Wang 《Contributions to Mineralogy and Petrology》2002,144(2):230-240
The Cretaceous gabbros in the Fujian coastal region, southeastern China, experienced different magmatic and tectonic processes associated with deformation of the Changle-Nanao shear zone. Group 1 gabbros (115 Ma) show marked LILE (e.g., Sr, Ba and K) and LREE enrichment, and HFSE (e.g., Ta, Nb, Zr and Hf) depletion, strongly suggesting an island-arc affinity. The parental magma of group 1 gabbros, arguably derived from an arc-related source mantle modified by previous subduction, rose into and interacted with the coexisting syntectonic granitic magma generated during the main stage of shear zone deformation, and produced the gabbro-diorite-granite complexes. Group 2 and 3 gabbros (106-95 Ma) possibly formed by coupling of the subduction-modified source mantle with part of undepleted mantle (e.g., Nb enrichment) in an extensional environment at the end of deformation. Their parental magmas did not undergo significant magma mixing but produced a cumulate nature. All the three groups of gabbros were contaminated by crustal material during the processes of intrusion and emplacement. 相似文献
5.
S. A. Goldberg 《Contributions to Mineralogy and Petrology》1984,87(4):376-387
Rocks enriched in iron oxide and mafic silicates are commonly present as minor volumes of Proterozoic anorthosite complexes. In the Laramie Range, Wyoming, anorthositic rocks, gabbros, and iron oxide ore have been chemically analyzed to determine if the spatial association is a result of genetic relationships between the rock types.Variations in abundances of REE, Th, Sc, and Sr in whole-rock and in mineral separates from anorthositic rocks provide evidence for the presence of trapped intercumulus liquid. Initial 87Sr/86Sr ratios in apatites separated from iron oxide ore (0.70535±0.00004) are analogous to initial 87Sr/86Sr ratios in Laramie Range anorthosite (0.70531 and 0.70537). In addition, REE abundances in calculated parental liquids for both anorthositic rocks and iron ore are similar, providing further evidence for a comagmatic relationship.Trace element and textural characteristics of spatially associated Laramie Range gabbros indicate that they are not mixtures of the trapped liquid and cumulus components which formed anorthositic rocks. It is suggested that gabbros are early differentiation products of a high-Al gabbroic magma which subsequently crystallized large volumes of plagioclase to produce the anorthosite massif. 相似文献
6.
U-Pb Zircon Geochronology and Geochemistry of Granitoids in the Douling Group in the Eastern Qinling 总被引：5，自引：0，他引：5
ZHANG Chengli LI Miao WANG Tao YUAN Honglin YAN Yunxiang LIU Xiaoming WANG Jianqi LIU YeThe Key Laboratory of Continental Dynamics Ministry of Education Department of Geology Northwest University Xi''an Shaanxi State Key Laboratory for Mineral Deposits Research Nanjing University Nanjing Jiangsu Institute of Geology Chinese Academy of Geological Sciences Beijing 《《地质学报》英文版》2004,78(1):83-95
LA-ICPMS U-Pb zircon dating of the Sanpinggou, Gangou and Fengzishan granitoids in the Douling Group of the Eastern Qinling yields ages of 760-685 Ma, which represents a strong tectono-magmatic event in the southern Qinling during the late Neoproterozoic. Geochemical data show that these intrusions have wide compositions ranging from minor gabbros through diorites to granodiorites. They are relatively enriched in LILE, poor in HFSE and strongly depleted in Nb and Ta, displaying affinities of Ⅰ-type granites formed in an active continental margin with oceanic subduction. In contrast to granitoids, gabbros and enclaves in the granitoids have higher REE abundances, relatively flat REE patterns, lower LILE, slightly higher HFSE and more depletion in Nb and Ta. All these suggest that the gabbros were formed by partial melting of the upper mantle above the subduction zone and the granitoids by the partial melting of the lower crust. Combined with regional geological data, the subduction-related granitoids in 相似文献
7.
This work presents new field and petrological data on a poorly known lower crustal section from the Alpine Jurassic ophiolites, the Pineto gabbroic sequence from Corsica (France). The Pineto gabbroic sequence is estimated to be ~1.5 km thick and mainly consists of clinopyroxene-rich gabbros to gabbronorites near its stratigraphic top and of troctolites and minor olivine gabbros in its deeper sector. The sequence also encloses olivine-rich troctolite and mantle peridotite bodies at different stratigraphic heights. The composition and the lithological variability of the Pineto gabbroic sequence recall those of the lower crustal sections at slow- and ultra-slow-spreading ridges. The gabbroic sequence considered in this study is distinct in the high proportion of troctolites and olivine gabbros, which approximately constitute 2/3 of the section. In particular, the lower sector of the Pineto gabbroic sequence shows the existence of large-scale fragments of the deepest oceanic crust displaying a highly primitive bulk composition. The mineral chemical variations document that the origin and the evolution of the Pineto gabbroic rocks were mostly constrained by a process of fractional crystallisation. The clinopyroxenes from the olivine gabbros and the olivine-rich troctolites also record the infiltration of olivine-dissolving, Cr2O3-rich melts that presumably formed within the mantle, into replacive dunite bodies. Cooling rates of the troctolites and the olivine gabbros were evaluated using the Ca in olivine geospeedometer. We obtained high and nearly constant values of ?2.2 to ?1.7 °C/year log units, which were correlated with the building of the Pineto gabbroic sequence through multiple gabbroic intrusions intruded into a cold lithospheric mantle. 相似文献
8.
对白云鄂博矿床大地构造环境的几点认识 总被引：1，自引：0，他引：1
分布于华北地台北缘的白云鄂博群厚万米，EW向展布长500km，宽20-50km，以碎屑岩为主，碳酸盐岩约占1/10。1997年，我们首次确定厚千余米的含矿岩系为海相火山沉积稀有金属碳酸岩—粗面岩；1982的，李继亮确定厚320m的次闪绿帘石岩（H15）为裂陷槽中的细碧角斑岩系。从而奠定了白云鄂博群属象谷沉积的基础。世界上许多富含轻稀土和铌和碱性岩、碳酸岩多产于裂谷系中。白云鄂博矿床中的特殊元素组合和稳定同位素组成只有裂谷带下的异常地幔才能提供。大量Sm-Nd同位素年龄资料说明白云鄂博矿床稀土成矿时代主要是中元古代，更证明了矿床成矿作用与裂谷发展的同步性。 相似文献
9.
Petros Koutsovitis 《Mineralogy and Petrology》2012,104(3-4):249-265
East Othris area consists of scattered ophiolitic units, as well as ophiolitic mélange occurrences, which encompass gabbroic rocks. These rocks have been affected by low-grade ocean floor metamorphism (T?<?350°C and P?<?8?kbar). Based on their petrography, mineral chemistry and geochemistry gabbroic rocks have been distinguished into gabbros and diorites, with the latter being divided into two groups. Gabbros seem to have been formed from moderate to high partial melting degrees (~8–25%) of a highly depleted mantle source, while group (1) diorites have been differentiated after variable fractionation processes (up to 30%). Group (2) diorites seem to have been derived from low partial melting degrees (~3%) of a fertile or moderately depleted mantle source and with extensive fractionation processes (~50%). Geochemical results suggest that partial melting processes occurred at relatively shallow depths, in the plagioclase-spinel stability field, while amphibole chemistry data indicate shallow level crystallization. Chondrite and PM-normalized patterns, Th/Yb, and Nb/Th ratios as well as mineral chemistry analyses show that gabbros and group (1) diorites (with relatively low PM-normalized Nb and Ta values and negative Ti anomalies) suggest subduction processes, while group (2) diorites are MORB or BAB related. Some gabbros have been characterised as high-Mg, being compositionally similar to picrites or boninites. Variability in extent of partial melting of the mantle source and the different geotectonic environment affinities are consistent with a supra-subduction zone (SSZ) origin of the east Othris ophiolites. The fact that IAT related rocks are more abundant in east rather than in west Othris may possibly be explained by a slab rollback model retreating to the east within the Pindos oceanic basin. 相似文献
10.
藏东南措美大火成岩省中OIB型镁铁质岩的全岩地球化学和锆石Hf同位素 总被引：6，自引：4，他引：2
西藏南东部新识别出来的措美大火成岩省的地幔柱头部物质成分尚未得到很好的约束。为探讨此问题,在全岩地球化学数据基础上,本文首次报道了藏东南措美大火成岩省中机布淌、打隆、措美和哲古错OIB型镁铁质岩的锆石Hf同位素和微量元素数据。本文报道的OIB型镁铁质岩包括碱性(组Ⅰ)和亚碱性(组Ⅱ)系列的辉长岩和辉绿岩,以岩墙或岩床的形式产出。这些镁铁质岩具有高的TiO2(2.61%～4.07%)和P2O5(0.32%～0.51%)含量,富集轻稀土元素和高场强元素,地球化学特征类似于OIB。全岩微量元素地球化学指标显示组Ⅰ样品没有或很少受到地壳混染,组Ⅱ样品经历了较高程度的地壳混染。组Ⅰ中一件样品(JBT03-1)具有变化范围大的锆石εHf(t)值(-4.8～+5.3),可能暗示其受到了地壳和/或岩石圈地幔物质的混染。本文结果表明锆石Hf同位素比全岩地球化学数据能够更为有效地识别基性岩浆是否受到地壳和/或岩石圈地幔物质混染。措美大火成岩省中的OIB型镁铁质岩样品(组Ⅰ和组Ⅱ),具有不同于俯冲带镁铁质岩和洋壳镁铁质岩的锆石稀土元素配分型式和锆石Ti温度,这可能是岩浆源区温度和成分不同的结果。综合考虑全岩地球化学和锆石Hf同位素指标,本文提出未受到地壳或岩石圈地幔混染的打隆镇辉长岩体(以组I中的DL01样品为代表)很可能代表了措美大火成岩省纯的地幔柱头部物质成分[87Sr/86Sr(t)=0.7047,εNd(t=+1.5,εHf(t=+2.1～+5.7]。这些成分与代表白垩纪Kerguelen地幔柱头部物质的Site 1138和Bunbury Casuarina玄武岩非常相似,可能指示措美大火成岩省中的OIB型镁铁质岩本身就是Kerguelen地幔柱头部物质发生减压熔融的产物。 相似文献
11.
Abstract Clinopyroxenes and garnets from 11 blueschist-facies Fe-rich eclogite samples from the Voltri Group show a wide range of chemical compositions. Detailed analyses of single pyroxene and garnet grains show wide and scattered chemical inhomogeneity, the KD (KD = (Fe2+ /Mg)Gt /(Fe2+ /Mg)Cpx ) ranges from 20 to 87 based on rim analyses only. The data obtained indicate that the mineral pairs never attained equilibrium under uniform P-T conditions and that the compositions of the metamorphic minerals were influenced mainly by the composition of the pre-metamorphic minerals and by topotactical reactions. 相似文献
12.
北部湾盆地福山凹陷古近系流沙港组二段泥岩中发育大面积巨厚辉长岩?地球化学分析表明,辉长岩具有中等TiO_2含量(2.15%~2.24%),较低MgO(5.77%~5.86%)、K_2O(1.18%~1.25%),P_2O_5(0.36%~0.39%)含量,且Na_2OK_2O,指示其类似于板内拉斑玄武岩。辉长岩ΣREE为105.61×10~(–6)~111.26×10~(–6),富集LREE,(La/Yb)_N=8.74~9.64,具有右倾型稀土配分模式;与原始地幔相比,富集Rb、Ba、Th、U等大离子亲石元素以及高场强元素Nb、Ta、Zr、Hf,呈现板内碱性玄武岩特征,是地幔物质上涌与上覆薄而年轻的岩石圈地幔相互作用的产物?结合LA-ICP-MS锆石U-Pb测年结果显示,辉长岩形成时间介于37~32 Ma,代表福山凹陷古近系辉长岩的侵位年龄,是古近纪岩石圈持续伸展环境下的产物?这对探讨福山凹陷以及中国东南部古近纪构造活动及岩浆演化具有重要的意义。 相似文献
13.
Mineralogy and geochemistry of banded iron formation and iron ores from eastern India with implications on their genesis 总被引：1，自引：0，他引：1
The geological complexities of banded iron formation (BIF) and associated iron ores of Jilling-Langalata iron ore deposits,
Singhbhum-North Orissa Craton, belonging to Iron Ore Group (IOG) eastern India have been studied in detail along with the
geochemical evaluation of different iron ores. The geochemical and mineralogical characterization suggests that the massive,
hard laminated, soft laminated ore and blue dust had a genetic lineage from BIFs aided with certain input from hydrothermal
activity. The PAAS normalized REE pattern of Jilling BIF striking positive Eu anomaly, resembling those of modern hydrothermal
solutions from mid-oceanic ridge (MOR). Major part of the iron could have been added to the bottom sea water by hydrothermal
solutions derived from hydrothermally active anoxic marine environments. The ubiquitous presence of intercalated tuffaceous
shales indicates the volcanic signature in BIF.
Mineralogical studies reveal that magnetite was the principal iron oxide mineral, whose depositional history is preserved
in BHJ, where it remains in the form of martite and the platy hematite is mainly the product of martite. The different types
of iron ores are intricately related with the BHJ. Removal of silica from BIF and successive precipitation of iron by hydrothermal
fluids of possible meteoric origin resulted in the formation of martite-goethite ore. The hard laminated ore has been formed
in the second phase of supergene processes, where the deep burial upgrades the hydrous iron oxides to hematite. The massive
ore is syngenetic in origin with BHJ. Soft laminated ores and biscuity ores were formed where further precipitation of iron
was partial or absent. 相似文献
14.
The SW Antalya Complex is an assemblage of Mesozoic carbonate platform, margin and ophiolitic rocks which record the formation and tectonic emplacement of a small Mesozoic ocean basin. The late Cretaceous ophiolitic rocks are located at two localities, namely the relatively intact Tekirova ophiolite to the east of Kemer zone and the dismembered Gödene ophiolite to the west of Kemer zone. The Tekirova (Antalya) ophiolite comprises harzburgitic tectonites, ultramafic to mafic cumulates, isotropic gabbros and sheeted dikes. Numerous isolated dikes, ranging in thickness from 5 cm to 10 m, intruded the crustal rocks at different structural levels. The isotropic gabbros are represented by gabbro, diorite and quartz diorite rocks with granular to ophitic–subophitic textures. The isolated dikes are characterized by dolerite, diabase and microdiorite with ophitic, intersertal and microgranular textures. These rocks exhibit tholeiitic to alkaline compositions. New geochemical data presented in this paper from the isolated dikes and isotropic gabbros suggest that there are three main types of parental basic magmas that form the oceanic crustal rocks of the Tekirova (Antalya) ophiolite. These are (1) IAT series which can be referred to the Group I isolated dikes and isotropic gabbros; (2) low-Ti boninitic series characterized by the Group II isolated dike and isotropic gabbros; and (3) OIB-type including the Group III isotropic gabbros. The geochemical evidence suggests that the crustal rocks of the Tekirova (Antalya) ophiolite were generated from a progressive source depletion from island arc tholeiites (IAT) to boninites. Therefore, a fore-arc tectonic setting seems likely for the generation of the crustal rocks from the Tekirova (Antalya) ophiolite in the southern branch of Neotethys during the Late Cretaceous. The OIB-type alkaline isotropic gabbros are thought to have resulted from either (1) a late-stage magmatic activity fed by melts that originated within an asthenospheric window due to slab break-off or (2) subduction of a ridge system which generated OIB source across the asthenospheric window that has been no influence of fluids from the subducted slab into the overlying mantle wedge, shortly before the emplacement of the Tekirova (Antalya) ophiolite onto the Tauride platform. 相似文献
15.
扬子陆块西南缘发育一系列中-新元古代岩浆岩,对认识扬子陆块构造演化具有重要意义.对会理地区天宝山组流纹岩和盐边地区辉长岩进行SHRIMP锆石U-Pb年代学、地球化学研究.天宝山组流纹岩时代为1 011.9±8.9 Ma,辉长岩时代为910.6±4.7 Ma.天宝山组流纹岩具有高硅、高FeOt/MgO、高钾等特征;稀土含量（∑REE=292×10-6~401×10-6）较高,表现出轻稀土富集重稀土弱亏损的特征[（La/Yb）N=1.77~6.74],Eu负异常明显（δEu=0.43~0.56）,与A型花岗岩相似;天宝山组流纹岩来自古老的地壳物质的部分熔融,形成于大陆裂谷环境.盐边群辉长岩稀土含量（∑REE=54×10-6~98×10-6）较低,轻重稀土分异较弱[（La/Yb）N=1.46~4.72],Eu具有轻微的异常（δEu=0.81~1.31）;岩石具有明显的Nb-Ta、Ti负异常,无Zr-Hf正异常;地球化学数据显示辉长岩来自被俯冲板片释放的流体/熔体交代的地幔楔部分熔融,形成于岛弧环境.两期岩浆活动指示了扬子西南缘1 000~910 Ma之间构造动力学背景发生了转变,由伸展背景转变为挤压背景. 相似文献
16.
The geochemical and zircon geochronological (U-Pb, SHRIMP-II) study of Mesoarchean gabbros of the South Vygozersky and Kamennoozersky greenstone structures of Central Karelia made it possible to distinguish four gabbro types: (1) Fe–Ti gabbro, 2869 ± 12 Ma, (2) gabbro compositionally close to tholeiitic basalts, 2857 ± 7 Ma, (3) leucogbabbro, 2840 ± 5 Ma; and (4) melanogabbro, 2818 ± 14 Ma. From the early to late gabbros, the rocks are depleted in Ti, Fe, V, Y, Zr, Nb, Hf, REE and enriched in Mg, Ca, Cr, Ni. According to the systematics (Condie, 2005), the Nb/Y, Zr/Y, Zr/Nb ratios in the studied Late Archean gabbros are close to those of primitive mantle, while the gabbros in composition are similar to those of plumederived ocean-plateau basalts. Their magma sources were derived from different mantle reservoirs. The leucogabbro and melanogabbro with similar εNd = +4 were derived from a depleted mantle source (DM). The gabbro close in composition to tholeiitic basalts and having the elevated positive εNd (+4.9) was derived from a strongly depleted mantle source. Insignificant admixture of crustal material or lithospheric mantle is inferred in a source of the Fe–Ti gabbro (with lowest εNd = +2.1). 相似文献
17.
《Geodinamica Acta》2013,26(1-2):21-35
The Voltri Massif underwent a polyphasic tectono-metamorphic evolution that records both the Alpine and part of the Apennine deformation events. So this is a key-area to investigate the relationships between Alpine and Apennine deformation events. This paper focus on the upper crustal deformations (UCD) that characterize the last stages of the tectonics of the Voltri Massif. In the Voltri Massif UCD are characterized by the superpositions of ductile, brittle-ductile and brittle structures that can be attributed to three main tectonic events (from D3 to D5). The oldest UCD event (D3) developed folds and reverse shear zones under ductile to brittle-ductile conditions. Main compressive NW-SE oriented regime characterized D3 event. Brittle-ductile to brittle reverse shear zones and important strike-slip/transpressive systems overprinted D3 structures. This D4 event was significant at the regional scale and occurred under main transpressive, NE-SW oriented, regime. The latest normal and transtensional brittle structures, that formed during UCD D5 event, locally reactivated the older structures. 相似文献
18.
Takeru Moriyama Mruganka K. Panigrahi Dinesh Pandit Yasushi Watanabe 《Resource Geology》2008,58(4):402-413
The major, trace and rare earth element (REE) composition of Late Archean manganese, ferromanganese and iron ores from the Iron Ore Group (IOG) in Orissa, east India, was examined. Manganese deposits, occurring above the iron formations of the IOG, display massive, rhythmically laminated or botryoidal textures. The ores are composed primarily of iron and manganese, and are low in other major and trace elements such as SiO2, Al2O3, P2O5 and Zr. The total REE concentration is as high as 975 ppm in manganese ores, whereas concentrations as high as 345 ppm and 211 ppm are found in ferromanganese and iron ores, respectively. Heavy REE (HREE) enrichments, negative Ce anomalies and positive Eu anomalies were observed in post‐Archean average shale (PAAS)‐normalized REE patterns of the IOG manganese and ferromanganese ores. The stratiform or stratabound shapes of ore bodies within the shale horizon, and REE geochemistry, suggest that the manganese and ferromanganese ores of the IOG were formed by iron and/or manganese precipitation from a submarine, hydrothermal solution under oxic conditions that occurred as a result of mixing with oxic seawater. While HREE concentrations in the Late Archean manganese and ferromanganese ores in the IOG are slightly less than those of the Phanerozoic ferromanganese ores in Japan, HREE resources in the IOG manganese deposits appear to be two orders of magnitude higher because of the large size of the deposits. Although a reliable, economic concentration technique for HREE from manganese and ferromanganese ores has not yet been developed, those ores could be an important future source of HREE. 相似文献
19.
Ten samples of blueschist facies eclogites occurring as dykes in the ultramafic rocks of the Voltri Group were analysed for eigth rare earth elements (REE). Their patterns are clearly different from those of cognate eclogites enclosed in ultramafic rocks and similar to those of the volcanic rocks dredged from the Mid-Atlantic Ridge (MAR). This similarity confirms both the tholeiitic nature of the magma injected into the Pennidic oceanic basement and metamorphosed to eclogite, and the immobile character of REE during metamorphism up to 10 Kbar and 450°C. Depletion of LREE vs HREE and a positive Eu anomaly in the coarse-grained central portions of the former dykes suggest their derivation from a mush consisting of pyroxene and plagioclase plus trapped superferrian liquid. The high total REE content and the flat pattern of the fine-grained eclogites occurring at the borders of the dykes are consistent with their derivation from a rapidly crystallized superferrian liquid. 相似文献
20.
Fe (136,900 ppm)- and Ti (28,540 ppm)-rich eclogites contained in the Voltri serpentinites show contents of metallic trace elements different from those of other eclogites described so far, both those of ophiolitic type and those included in ultramafic rocks. The Voltri eclogites are enriched in Mn (1,894 ppm), V (610 ppm), and Co (75 ppm) and depleted in Cr (110 ppm), Ni (56 ppm), and Zr (46 ppm) in comparison with other occurrences. The analyzed samples are: twelve flaser-eclogites, four fine-grained bimineralic eclogites and three eclogites showing an advanced degree of retrometamorphism toward greenschist facies. The given average values (in ppm) are based on nineteen analyzed samples. This trace-element content is believed to reflect the highly fractionated tholeiitic character of the eclogites and suggests that the Voltri rocks originated from the isochemical metamorphism of ferrogabbros which were probably intruded into the serpentinized lherzolites of a mid-oceanic ridge at the time of the opening of the Pennidic trough. 相似文献