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黄智龙 《大地构造与成矿学》1997,21(1):24-31
在已有云南鸡街碱性超基性杂岩体地质、地球化学资料基础上，本文利用岩石学混合计算等方法对杂岩体源区成分、结晶分异过程进行模拟。结果表明，鸡街杂岩体来源于亏损地幔；岩体中相对早期碱性超基性岩（主体岩石：霞霓纳辉岩、霓霞岩和磷霞岩）为很少或没有受到上部地壳物质污染的幔源岩浆结晶分异作用产物；晚期碱性中性岩（脉岩：钠霞正长岩和霓辉钠长斑岩）为幔源岩浆（与碱性超基性岩同源）演化过程中发生岩浆液态不混淆作用产物。 相似文献
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1958年袁棨林在我国北部一地槽区曾注意到有两类超基性岩体。第Ⅰ类有橄长岩-异剥辉长岩分异脉岩(以下简称分异脉岩)的岩体,其造矿铬尖晶石为较富铝的富铬尖晶石亚种和富铁富铬尖晶石亚种,组成低品位冶金级矿石;第Ⅱ类为无分异脉岩的岩体,其中合富铬贫铝的铬铁矿亚种和富铁铬铁矿亚种,组成高品位冶金级矿石。它们虽然都是镁质超基性岩,同样是以斜辉辉撖岩为主的纯橄榄岩-辉橄岩杂岩体,而且都显示了较强的动力分异作用,只是由于出现或不出现与晚期岩浆铬铁矿有成因关系的分异脉岩,而使造矿铬失晶石成分有明显地不同。 相似文献
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青海南山沟后岩浆杂岩体锆石U-Pb年代学、岩石成因及其地质意义 总被引：1，自引：0，他引：1
青海南山构造带是衔接宗务隆构造带、南祁连构造带和西秦岭造山带的重要结合带。沟后岩浆杂岩体位于青海南山构造带东段,主要由辉长岩、辉长闪长岩、石英闪长岩、花岗闪长岩组成。本文对沟后岩浆杂岩体进行了详细的岩石学、岩石地球化学和LA-ICP-MS锆石U-Pb同位素年代学研究。结果表明,辉长岩、辉长闪长岩、石英闪长岩、花岗闪长岩及暗色微粒包体的结晶年龄分别为248.8±2.6 Ma、243.2±2.1 Ma、243.1±0.9 Ma、244.0±2.1 Ma和249±3 Ma。辉长岩富铁、镁,贫碱;辉长闪长岩高铝、富钙和钠,二者均为钙碱性岩类。石英闪长岩和花岗闪长岩为准铝-弱过铝质高钾钙碱性岩,暗色微粒包体属钙碱性-碱性岩系列。不同岩石类型均表现为富集大离子亲石元素(Cs、Rb、K)和Pb,亏损高场强元素(Nb、Ta、Ti)和P、Ba负异常;稀土元素配分曲线均具有轻重稀土分异的右倾特征,具弱-中等负Eu异常。岩相学和岩石地球化学特征表明沟后岩浆杂岩体具壳幔岩浆混合特征,暗示其可能形成于由俯冲流体交代地幔楔部分熔融的幔源岩浆底侵作用下的构造环境。辉长岩为幔源岩浆经分离结晶的产物,辉长闪长岩为幔源岩浆经分异演化并混染少量壳源岩浆的产物;中基性岩浆与壳源中酸性岩浆发生混合并经历一定的分异演化过程形成了石英闪长岩和花岗闪长岩。结合区域地质资料分析认为,沟后岩浆杂岩体可能代表了研究区早三叠世晚期-中三叠世早期宗务隆洋向南消减作用相关的构造岩浆事件。 相似文献
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应用电子探针技术研究北京密云放马峪铬铁矿床成因——来自含铬尖晶石矿物化学的证据 总被引：1，自引：1，他引：0
似层状铬铁矿床长期以来被认为是岩浆分异成因,但近年来有学者提出其中个别产在蛇绿岩中。本文选择北京放马峪似层状铬铁矿床中纯橄岩、辉橄岩和辉石岩中不同类型的含铬尖晶石进行了电子探针分析。研究表明,岩浆早期的纯橄岩和辉橄岩中的铬尖晶石富铬(Cr2O3平均43.32%),而岩浆晚期辉石的结晶消耗了大量Cr3+,由于氧逸度的升高,在辉石岩的单斜辉石中出溶贫铬的铬磁铁矿(Cr2O3平均10.32%)和富铝尖晶石(Cr2O3平均15.77%)。与世界上不同类型铬尖晶石的矿物化学特征进行对比,可以认为放马峪铬铁矿床是产在阿拉斯加型岩体中的早期岩浆矿床,而与蛇绿岩无关。本文对放马峪铬铁矿床成因和成矿专属性的限定,为这类镁铁-超镁铁岩体的铬、铜镍、铂族元素的找矿勘查提供了依据。 相似文献
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西南天山哈拉达拉岩体的锆石SHRIMP年代学及地球化学研究 总被引：15，自引：6，他引：9
西南天山哈拉达拉侵入体由橄长岩、橄榄辉长岩和辉长岩组成,橄长岩和橄榄辉长岩具有典型的堆晶结构,堆晶矿物以斜长石和橄榄石为主。辉石、角闪石和金云母主要为堆晶间隙矿物。辉长岩发育辉长—辉绿结构。结晶分异作用在岩浆演化过程中起重要作用。对从辉长岩中分选出来的锆石进行的SHRIMP年代学研究表明,辉长岩形成于308.3±1.8Ma （MSWD=0.86,n=15）。哈拉达拉岩体稀土元素配分模式与E-MORB相似,具有高Rb、Cs、Ba及Sr的特点,87Sr/86Sr初始比值0.7040~0.7050。这些特征表明,岩浆源区具有富集地幔的特征(古南天山洋俯冲流体交代形成了富集地幔)。根据平坦的稀土元素配分模式以及Gd、Sm、Nb、Zr等微量元素的地球化学行为判别,岩浆源区岩石为含角闪石的尖晶石二辉橄榄岩。批式熔融模拟计算显示,地幔岩10%~15%的部分熔融能够形成哈拉达拉岩体的母岩浆。母岩浆通过48%~50%的结晶分异作用则能够形成哈拉达拉岩体。早期结晶的橄榄石和斜长石通过堆晶作用形成橄长岩和橄榄辉长岩,剩余岩浆结晶形成辉长岩。 相似文献
6.
碱性-超基性杂岩体主要分布于俄罗斯东部稳定地质构造中,并经历了中生代-新生代的构造-岩浆作用.这些杂岩体局限于长期活动的深断裂带中.一些岩体由多期岩浆岩组成,并逐渐形成岩浆源构造(为1500~1000Ma).在该构造中,于前寒武纪或古生代形成的超镁铁质核被新生代或中生代碱性岩、花岗岩类和二长岩所穿切.碱性-超镁铁质岩体具有完好的同心带状构造,由不含黄长石的钙-碱性至碱性岩组成(作为一种规律).碱性-超镁铁质火山岩和侵入岩由碱性苦橄岩、黄橄玄霞岩、金伯利岩和超基性似长岩、玄武角闪岩及霞岩组成. 相似文献
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位于东昆仑造山带东段的浪木日铜镍钴多金属矿床，在新近勘查工作中又圈出独立的铂矿体，对该矿床成矿特征的进一步研究有助于指导勘查找矿.通过矿床地质特征分析，结合含矿橄辉岩主微量元素、Sr‐Nd同位素及其中橄榄石、云母主量元素测试，以及黑云母花岗岩锆石U‐Pb年代学及岩石地球化学特征研究，探讨了浪木日矿床成矿特征、成矿时代及矿床成因.含矿橄辉岩中橄榄石属贵橄榄石(Fo值为86.72～88.39)，云母为金云母，其均为幔源岩浆作用产物；含矿橄辉岩稀土元素具右倾型的配分模式，富集Cs、Rb、U等元素，εNd(t)值为0.66～2.66，暗示其形成过程中经历了地壳混染.获得黑云母花岗岩U-Pb年龄为414.5±8.8 Ma，其具弧岩浆地球化学特征，(87Sr/86Sr)i(0.718 609～0.719 177)、εNd(t)值(1.28～5.36)显示其为壳幔岩浆混合作用产物.本研究认为浪木日铜多金属矿床具叠加成矿特征，在450～439 Ma形成与橄辉岩有关的铜镍钴铂钯矿体的基础上，叠加... 相似文献
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DONG Guochen MO Xuanxue ZHAO Zhidan GUO Tieying WANG Liangliang CHEN Tao 《《地质学报》英文版》2005,79(6):787-794
Abstract Abundant small mafic intrusions occur associated with granitoids along the Gangdisê magmatic belt. In addition to many discrete gabbro bodies within the granitoid plutons, a gabbro‐pyroxenite zone occurs along the southern margin of the Gangdisê belt to the north of the Yarlung Zangbo suture. The mafic intrusion zone spatially corresponds to a strong aeromagnetic anomaly, which extends ～1400 km. The mafic intrusions consist of intermittently distributed small bodies and dikes of gabbro and dolerite with accumulates of pyroxenite, olivine pyroxenite, pegmatitic pyroxenite and amphibolite. Much evidence indicates that the Gangdisê gabbro‐pyroxenite assemblage is most likely a result of underplating of mantle‐derived magma. Detailed field investigation and systematic sampling of the mafic rocks was conducted at six locations along the Lhasa‐Xigazê segment of the mafic intrusive zone, and was followed by zircon SHRIMP II U‐Pb dating. In addition to the ages of two samples previously published (47.0±1 Ma and 48.9±1.1 Ma), the isotopic ages of the remaining four gabbro samples are 51.6±1.3 Ma, 52.5±3.0 Ma, 50.2±4.2 Ma and 49.9±1.1 Ma. The range of these ages (47–52.5 Ma) provide geochronologic constraints on the Eocene timing of magma underplating beneath the Gangdisê belt at ca. 50 Ma. This underplating event post‐dated the initiation of the India‐Eurasia continental collision by 15 million years and was contemporaneous with a process of magma mixing. The SHRIMP II U‐Pb isotopic analysis also found several old ages from a few zircon grains, mostly in a range of 479–526 Ma (weighted average age 503±10 Ma), thus yielding information about the pre‐existing lower crust when underplating of mafic magma took place. It is believed that magma underplating was one of the major mechanisms for crustal growth during the Indian‐Eurasia collision, possibly corresponding in time to the formation of the 14–16 km‐thick “crust‐mantle transitional zone” characterized by Vp = 6.85–6.9 km/s. 相似文献
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赣北程浪超基性-基性杂岩特征及其Sm-Nd等时线年龄 总被引：4，自引：1，他引：3
扬子古地台板块东南前缘发育一系列晚前寒武纪移置地体。本文着重论述了彭庐地体与障公山地体间深断裂带内的铁质超基性－基性杂岩特征。主要岩石类型有纯橄榄岩、二辉橄榄岩、斜辉橄榄岩、含长橄榄辉石岩、角闪岩及辉长岩、辉绿岩。其全岩钐钕等时线年龄为８２８．６±２７．９Ｍａ,属晋宁运动产物。杂岩体产状与地体边界深断裂产状一致,与晚前寒武纪围岩地层产状斜交。杂岩体片理产状与围岩轴面流劈理产状一致,被后寒武纪地台沉积盖层不整合覆盖。推测,地体在拼贴挤压过程中,玄武岩浆从上地幔上升过程中携带了大量超基性岩块沿深断裂侵入上升就位。 相似文献
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Chao-Nan Hu 《International Geology Review》2018,60(9):1073-1097
The northern margin of the North China Craton (NCC) was an active convergent margin during Palaeozoic and preserves important imprints of magmatic and metasomatic processes associated with oceanic plate subduction. Here, we investigate the mafic–ultramafic rocks in the Xiahabaqin–Sandaogou complexes from the northern NCC including pyroxenite, hornblendites, hornblende gabbro, and their rodingitized counterparts within a serpentinite domain. We present petrological, zircon U–Pb geochronological, and geochemical data to constrain the nature and timing of the magmatic and metasomatic processes in the subduction zone mantle wedge. The rock suites investigated in this study are characterized by low contents of SiO2, Na2O, and K2O, with high CaO, FeO, Fe2O3, and MgO. The rodingitized rocks show markedly high CaO and lower MgO compared to their ultramafic protolith, suggesting extensive post-magmatic infiltration of Ca-rich, Si-poor fluids derived by serpentinization of mantle peridotite. The enrichment of large ion lithophile and light rare earth elements such as Ba, Sr, K, La, and Ce with relative depletion of high field strength elements like Nb, Ta, Zr, and Hf in the ultramafic rocks collectively suggest metasomatism of a fore-arc mantle wedge by fluids released through dehydration of subducted oceanic slab and subduction-derived sediments. Dehydration and decarbonation leading to metasomatic fluid influx and serpentinization of mantle wedge peridotite account for the enriched geochemical signatures for the rodingitized rocks. The zircon grains in these rocks show textures indicating magmatic crystallization followed by fluid-controlled dissolution–precipitation. Magmatic zircons from altered pyroxenite, hornblendite, and rodingitized pyroxenite in Xiahabaqin yield protolith crystallization ages peaks at 396 Ma and 392 Ma and metasomatic grains show ages of 386 Ma, 378 Ma, and 348 Ma. The zircons from hornblendite and basaltic trachyandesite indicate protolith emplacement during 402–388 Ma. Metasomatic zircon grains from rodingitized hornblende gabbro in Sandaogou complex show a wide range of ages as 412 Ma, 398 Ma, 383 Ma, and 380 Ma. The common magmatic zircon ages peaks at 398–388 Ma in most of the rocks suggest a similar time for magma crystallization in the Xiahabaqin and Baiqi during Middle Devonian. Subsequently, repeated pulses fluids and melts resulted in metasomatic reactions in mantle wedge until early Permian. The Lu–Hf analysis of the zircon grains from these rocks display markedly negative εHf(t) values ranging from ?22.4 to ?7.7, suggesting magma derivation from an enriched, hydrated lithospheric mantle through fluid–rock interaction and mantle wedge metasomatism. Rodingitization processes are associated with exhumation of ultramafic mantle wedge rocks within a serpentinized subduction channel close to the subducted slab in response to slab roll back in a long-lasting subduction regime. This study offers insights into magmatic and metasomatic processes of ultramafic rocks in the fore-arc mantle wedge which were exhumed and accreted to an active continental margin during the southward subduction of the Palaeo-Asian oceanic lithosphere beneath the NCC. 相似文献
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湘东南汝城盆地火山岩的元素地球化学及源区性质讨论 总被引：12，自引：4，他引：12
湘东南汝城盆地火山岩系由辉绿岩、玄武岩和玄武质火山碎屑岩组成 ,属于低钾拉斑玄武岩系。玄武岩全岩K Ar年龄为 ( 12 8 4± 4 2 )Ma ,辉绿岩全岩K Ar年龄为 ( 112 1±3 2 )Ma。元素地球化学分析表明火山岩系具有同一岩浆源区 ,其形成以部分熔融方式为主。岩石微量元素出现大离子亲石元素Rb、Ba、Th、U的富集和高场强元素Ta、Nb、Ti的亏损。强不相容元素含量的比值表明岩浆源区明显偏离原始地幔组分 ,具有富集型地幔的特征。岩浆源区主要受到地壳物质混染以及来自消减残留板片析出流体的交代改造作用。 相似文献
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牛鼻子梁镁铁质-超镁铁质杂岩体岩石特征 总被引：1，自引：1，他引：0
牛鼻子梁岩体位于柴达木地块的北缘,出露面积约8 km2,平面形态呈长条状,主要由斜长二辉橄榄岩、斜长单辉橄榄岩、角闪二辉橄榄岩、角闪橄榄岩、角闪橄榄二辉岩、黑云母化二辉岩、角闪辉石岩、橄榄辉石角闪石岩、角闪橄榄辉长岩、细粒辉长岩、似斑状辉长岩、暗色辉长岩、辉长岩、淡色辉长岩、石英闪长岩和英云闪长岩组成。文章通过岩石学、矿物学、地球化学研究,得到锆石U-Pb年龄为（361.5±1.2） Ma,Sm-Nd等时线年龄为（347±26） Ma。研究认为,牛鼻子梁基性-超基性岩体含矿岩石产于大陆边缘环境。岩体形成于泥盆纪晚期。岩浆分异充分,岩石类型丰富,岩浆演化过程中主要发生了橄榄石和斜长石的分离结晶/堆晶作用。岩体的母岩浆应属于拉斑玄武岩质岩浆。从目前发现的矿化情况来看,牛鼻子梁基性-超基性杂岩体为含矿岩体,有很好的找矿前景。 相似文献
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Summary The Shillong Plateau of northeastern India hosts four Early Cretaceous (105–107Ma) ultramafic-alkaline-carbonatite complexes (UACC), which have been associated with the Kerguelen plume igneous activity. Petrological and geochemical characteristics of one of these UACC, the Sung Valley, are presented. The Sung Valley UACC was emplaced in to the Proterozoic Shillong Group of rocks and consists of ultramafics (serpentinized peridotite, pyroxenite, and melilitolite), alkaline rocks (ijolite and nepheline syenite), and carbonatites. Serpentinized peridotite, pyroxenite, and ijolitic rocks form the major part of the complex, the others constitute less than 5% of the total volume. Ijolite and melilitolite intrude peridotite and pyroxenite, while nepheline syenite and carbonatite intrude the ultramafic rocks as well as ijolite. Mineralogically, the carbonatites are classified as calcite carbonatite with minor apatite, phlogopite, pyrochlore and ilmenite. The serpentinized peridotites are wehrlitic. Chemical compositions of the silicate rocks do not show a distinct co-genetic relationship amongst them, nor do they show any geochemical relationships with the carbonatites. No noticeable fractionation trend is observed on the chemical variation diagrams of these rocks. It is difficult to establish the genetic evolution of the Sung Valley UACC through fractional crystallization of nephelinitic magma or through immiscible liquids. On the basis of petrological and geochemical data and previously published isotopic results from these rocks, it is suggested that they have been derived from a primary carbonate magma generated by the low-degree melting of a metasomatized mantle peridotite. 相似文献
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河北省赤城县小张家口超基性岩体主要特征和时代 总被引：6，自引：2，他引：6
小张家口超基性岩体是华北板块北缘超基性岩带的一个典型岩体，岩相分带明显，由透辉岩、闪辉岩、二辉岩和纯橄岩组成，主要矿物组成包括透辉石、贵橄榄石、角闪石等。化学成分上富ＦｅＯ、ＣａＯ而贫ＭｇＯ，ｍ／ｆ平均２．２１，属铁质或富铁质超基性岩。稀土分布形式为轻稀土富集型，具不显著的负铕异常，微量元素以富含不相容元素Ｒｂ、Ｔｉ、Ｓｒ、Ｖ等而贫Ｃｒ、Ｃｏ、Ｎｉ等相容元素为特征。Ｓｍ－Ｎｄ等时年龄１８３７Ｍａ，Ｎｄ（ｔ）为十１０．７２。该岩体由亏损型地幔部分熔融所产生的岩浆经结晶分异作用而形成。 相似文献
18.
新疆磁海铁矿区镁铁质岩及正长岩锆石U-Pb年代学、岩石地球化学特征:对成岩、成矿作用的制约 总被引：4，自引：1，他引：3
对新疆磁海铁矿区镁铁-超镁铁质岩与铁成矿关系、正长岩与镁铁质岩关系的解剖,是认识磁海矿区成岩、成矿过程及构造背景的关键。本文利用SIMS锆石U-Pb测年法,获得磁海辉绿岩、辉长辉绿岩、磁南辉长岩、磁海北角闪石英正长岩的206Pb/238U-207Pb/235U谐和年龄分别为275.1±2.2Ma、281.9±3.2Ma、273.0±1.9Ma和273.0±1.8Ma,这与北山乃至北疆地区主要含铜镍-钒钛磁铁矿的镁铁-超镁铁质岩年龄一致。岩石地球化学特征研究显示,从辉石岩到辉长岩,再到辉绿岩,经历了Ti逐渐富集、Mg#和m/f值先增加后降低的过程,角闪石英正长岩具有A型花岗岩特征,与辉长岩、辉绿岩在成因上存在互补关系。综合年代学和地球化学特征,磁南辉石岩、辉长岩、磁海辉绿岩、辉长辉绿岩以及磁海北边的角闪石英正长岩为同源岩浆演化的产物,岩浆演化过程中受地壳混染作用微弱,在岩浆演化的早期,磁铁矿的结晶分离主导着岩浆成分的改变,当岩浆演化到辉长岩阶段,岩浆开始以结晶分异作用为主;磁铁矿的分离结晶时间早于钛铁矿,岩浆型的金属硫化物为磁铁矿和钛铁矿结晶过渡阶段的产物。磁海镁铁-超镁铁质岩石在成岩及成矿作用上可能与在时间和空间上相邻近的塔里木早二叠世大火成岩省有密切关系。 相似文献
19.
Origin of the UG2 chromitite layer, Bushveld Complex 总被引：3，自引：0，他引：3
Chromitite layers are common in large mafic layered intrusions.A widely accepted hypothesis holds that the chromitites formedas a consequence of injection and mixing of a chemically relativelyprimitive magma into a chamber occupied by more evolved magma.This forces supersaturation of the mixture in chromite, whichupon crystallization accumulates on the magma chamber floorto form a nearly monomineralic layer. To evaluate this and othergenetic hypotheses to explain the chromitite layers of the BushveldComplex, we have conducted a detailed study of the silicate-richlayers immediately above and below the UG2 chromitite and anotherchromitite layer lower in the stratigraphic section, at thetop of the Lower Critical Zone. The UG2 chromitite is well knownbecause it is enriched in the platinum-group elements and extendsfor nearly the entire 400 km strike length of the eastern andwestern limbs of the Bushveld Complex. Where we have studiedthe sequence in the central sector of the eastern Bushveld,the UG2 chromitite is embedded in a massive, 25 m thick plagioclasepyroxenite consisting of 60–70 vol. % granular (cumulus)orthopyroxene with interstitial plagioclase, clinopyroxene,and accessory phases. Throughout the entire pyroxenite layerorthopyroxene exhibits no stratigraphic variations in majoror minor elements (Mg-number = 79·3–81·1).However, the 6 m of pyroxenite below the chromitite (footwallpyroxenite) is petrographically distinct from the 17 m of hangingwall pyroxenite. Among the differences are (1) phlogopite, K-feldspar,and quartz are ubiquitous and locally abundant in the footwallpyroxenite but generally absent in the hanging wall pyroxenite,and (2) plagioclase in the footwall pyroxenite is distinctlymore sodic and potassic than that in the hanging wall pyroxenite(An45–60 vs An70–75). The Lower Critical Zone chromititeis also hosted by orthopyroxenite, but in this case the rocksabove and below the chromitite are texturally and compositionallyidentical. For the UG2, we interpret the interstitial assemblageof the footwall pyroxenite to represent either interstitialmelt that formed in situ by fractional crystallization or chemicallyevolved melt that infiltrated from below. In either case, themelt was trapped in the footwall pyroxenite because the overlyingUG2 chromitite was less permeable. If this interpretation iscorrect, the footwall and hanging wall pyroxenites were essentiallyidentical when they initially formed. However, all the modelsof chromitite formation that call on mixing of magmas of differentcompositions or on other processes that result in changes inthe chemical or physical conditions attendant on the magma predictthat the rocks immediately above and below the chromitite layersshould be different. This leads us to propose that the Bushveldchromitites formed by injection of new batches of magma witha composition similar to the resident magma but carrying a suspendedload of chromite crystals. The model is supported by the commonobservation of phenocrysts, including those of chromite, inlavas and hypabyssal rocks, and by chromite abundances in lavasand peridotite sills associated with the Bushveld Complex indicatingthat geologically reasonable amounts of magma can account foreven the massive, 70 cm thick UG2 chromitite. The model requiressome crystallization to have occurred in a deeper chamber, forwhich there is ample geochemical evidence. KEY WORDS: Bushveld complex; chromite; crystal-laden magma; crustal contamination; magma mixing; UG2 chromitite 相似文献
20.
汉南金水-青泥坑镁铁层状杂岩体位于扬子板块北缘汉南地体东北部,岩体侵位于中元古代西乡群。岩体出露面积大于500km~2。杂岩体主要由镁铁质辉长岩和部分超镁铁质辉石岩和橄榄岩组成。按层状岩序和岩石类型可以划分为上、下两个岩带,即由辉长岩类组成的上部带和由辉石岩-橄榄岩-粗粒蚀变辉长岩组成的下部岩带。研究表明,岩体的岩石化学、矿物化学和微量元素地球化学与层状岩序的演变相一致。韵律层发育部位,矿物组分多次重复出现,反映了形成杂岩体的岩浆有过多次侵位活动。还表明,层状岩序稀土总量和(La/Yb)_N值随层序增高而增加分馏趋势的一般规律。系统阐述了杂岩体各类岩石铂族元素分配特征。初步确定了铂矿化与铜镍矿化产出部位,讨论了铂族元素成矿作用问题。报告在分析了杂岩体产出的地质构造环境的基础上,探讨了杂岩体原始岩浆源的性质,同时估算了部分熔融程度。 相似文献