华夏地块:一个由古老物质组成的年轻陆块

对华夏地块三个主要前寒武纪地质体出露区变质岩的详细锆石年代学的综合分析显示,华夏地块大致可以被分成武夷山区和南岭-云开区。武夷山区由古元古代核和新元古代（形成于730-820 Ma）的盖层组成,构成华夏地块最老的古陆,在其深部很可能还存在一个新太古代基底。新元古代的沉积物主要来自武夷微古陆本身。南岭与云开具有相似的前寒武纪地壳组成,它们主要是由新元古代形成的沉积物夹少量火山岩组成。这些沉积物质中包含了非常古老的中太古代和新太古代组分,甚至古太古代组成。Grenville期和中元古代组分是其中最丰富的。这些组分在华夏没有对应出露的岩石,说明它们主要来自另外一个曾经与华夏相邻的陆块。该陆块很可能是东印度－东南极大陆。南岭－云开区最初可能是Rodinia超大陆裂解时形成的一个裂谷盆地,加里东的造山运动使盆地中的沉积物挤压、褶皱和隆起,与武夷陆块共同构成了一个新的年轻的大陆     

若尔盖与西秦岭地震反射岩石圈结构和盆山耦合

松潘地块北缘的若尔盖盆地与西秦岭造山带相接触,构成青藏高原东北缘典型的新生代盆山构造.其岩石圈结构与深部构造关系,记录了青藏高原东北缘板块碰撞的深部过程,同时又关联着若尔盖盆地油气远景的评价.2004年秋冬季,我们完成了第一条跨越若尔盖盆地和西秦岭造山带的深地震反射剖面.整个剖面全长254 km,分5段完成,其中第2段剖面（简称SP04_2）横过盆山结合部位.SP04_2剖面首次揭示若尔盖盆地－西秦岭造山带盆山结合部位的岩石圈结构,发现了若尔盖盆地和西秦岭造山带下地壳均以北倾为主的强反射特征,提供出若尔盖盆地下地壳整体向西秦岭造山带俯冲的地震学证据,揭示了若尔盖盆地和西秦岭造山带在挤压构造体系下形成的深部构造关系.而近于平的Moho反射特征又反映出两者在造山后期经历了强烈的伸展作用.     

The Weixi High-silica Granitoids in the Central Sanjiang Orogenic Belt, Southwest China: Implications for Growth of the Continental Crust

High-silica granitoids record the formation and evolution of the continental crust. A new intrusive complex has been recognized among silicic volcanic rocks of the Weixi arc, Southwest China. The intrusions consist of granites, granitic porphyries, and granodiorites. Zircon U-Pb age data indicate that the Weixi granitoids formed at 248–240 Ma and were coeval with silicic volcanic rocks of the Weixi arc. The Weixi granitoids are enriched in Rb, Th, and U, depleted in Ba, Sr, Nb, Ta, and Ti, and have high light/heavy rare earth element ratios and slightly negative Eu anomalies. The Weixi granitoids have negative εNd(t) values (?9.8 to ?7.8) and negative zircon εHf(t) values (?12.02 to ?5.11). The geochemical and isotopic features suggest the Weixi granitoids were derived by partial melting of ancient crustal material. The Weixi granitoids and silicic volcanic rocks were derived from the same magma by crystal accumulation and melt extraction, respectively, and they record the formation of a continental arc in the central Sanjiang orogenic belt.     

Refining accretionary orogen models for the Tasmanides of eastern Australia

The well-known southwest-to-northeast younging of stratigraphy over a present-day cross strike distance of >1500 km in the southern Tasmanides of eastern Australia has been used to argue for models of accretionary orogenesis behind a continually eastwards-rolling paleo-Pacific plate. However, these accretionary models need modification, since the oldest (ca 530 Ma) outcrops of Cambrian supra-subduction zone rocks occur in the outboard New England Orogen, now ～900 km east of the next oldest (520–510 Ma) supra-subduction zone rocks. This is not consistent with simple, continuous easterly rollback. Instead, the southern Tasmanides contain an early history characterised by a westwards-migrating margin between ca 530 and ca 520 Ma, followed by rapid eastwards rollback of the paleo-Pacific plate from 520 to 502 Ma that opened a vast backarc basin ～2000 km across that has never been closed. From the Ordovician through to the end of the Carboniferous, the almost vertical stacking of continental margin arcs (within a hundred kilometres of each other) in the New England Orogen indicates a constant west-dipping plate boundary in a Gondwana reference frame. Although the actual position of the boundary is inferred to have undergone contraction-related advances and extension-related retreats, these movements are estimated to be ～250 km or less. Rollback in the early Permian was never completely reversed, so that late Permian–Triassic to Cretaceous arcs lie farther east, in the very eastern part of eastern Australia, with rifted fragments occurring in the Lord Howe Rise and in New Zealand. The northern Tasmanides are even more anomalous, since they missed out on the middle Cambrian plate boundary retreat seen in the south. As a result, their Cambrian-to-Devonian history is concentrated in a ～300 km wide strip immediately west of Precambrian cratonic Australia and above Precambrian basement. The presence in this narrow region of Ordovician to Carboniferous continental margin arcs and backarc basins also implies a virtually stationary plate boundary in a Gondwana frame of reference. This bipolar character of the Tasmanides suggests the presence of a segmented paleo-Pacific Plate, with major transform faults propagating into the Tasmanides as tear faults that were favourably oriented for the formation of local supra-subduction zone systems and for subsequent intraplate north–south shortening. In this interpretation of the Tasmanides, Lower–Middle Ordovician quartz-rich turbidites accumulated as submarine fan sequences, and do not represent multiple subduction complexes developed above subduction zones lying behind the plate boundary. Indeed, the Tasmanides are characterised by the general absence of material accreted from the paleo-Pacific plate and by the dominance of craton-derived, recycled sedimentary rocks.     

大别造山带钾氩年龄的解释—差异上升的地块

根据冷却年龄理论和大别造山带变质岩K-Ar表面年龄的平面分布,指出这些年龄既不代表岩石形成事件,也不简单地反映后期热事件,而代表岩石经剥蚀隆起温度下降到该矿物封度温度以来的时间,即反映地区的构造隆起历史。现有资料说明大别造山带整体在印支期开始隆起,但中部罗田—英山一带则隆起较快或地热增温率高,因而表现出年轻(燕山期)的表面年龄。     

漳州-华安“地震窗”及其机制

漳州-华安是一个中强地震活动区,现今小震活动频繁。本文分析该区历史和现今地震活动特点,发现该区地震活动性涨落与闽台强震活动存在一定的相关性,因而得出该区是一个“地震窗”的认识。进而对“地震窗”的形成条件进行讨论,认为该区“地震窗”的形成是与其深部热作用所产生的向上垂直作用力紧密相关     

华北块体(地台)北缘几个地质问题的探讨及其成矿作用

本文以卫星图象信息为依据,结合野外调研,提出并确定了华北块体北缘存在:块体缝合线,褶皱-逆掩断层带,后孤碰撞带(断裂带),台槽过渡带,岩浆弧,以及燕山-喜山期的NNE向岩浆活动带、断陷带(断陷盆地)等双重构造的新认识。并在此基础上,对华北块体北缘与深成岩浆岩,燕山期岩浆活动带(包括火山岩带)有关的铀矿化作用的独特构造环境及“岩浆”型,断陷带中和面型等主要铀矿床成矿模式和铀成矿带的划分及其划分依据作了研究和探讨。并以铀矿床的实例作为佐证。     

台北盆地构造特征及形成机制探讨

台北盆地位于台湾造山带的北部,它的形成有其特殊的机制而不同于一般意义上由于造山带的垮塌直接导致的盆地。钻井、地震勘探等资料表明,控制盆地形成的山脚断层并不是一条完整的正断层,而是由 3个段落组成,每个段落控制 1个沉积中心,彼此之间没有沟通。山脚断层各段落的活动性并不相同,向NE方向随时间逐渐增强,目前最为活动的段落集中在中段和北段,南段已不活动。台北盆地并不是一个孤立发育的盆地,是与金山断层东南的大屯火山群同时陷落的,具有一致的地球物理场背景、沉降规模以及正断层活动,广义的台北盆地从沉降范围和机制上还应该包括金山断层以南的大屯火山群。盆地周围发育了一系列的火山 (群),由于盆地的发育是紧随这些火山主要活动之后的,盆地的形成与周围火成活动有着必然联系,一些地球物理资料和盆地内的构造发育及沉积迁移特征表明,台北盆地的发育是深部岩浆体的冷却收缩所致。台北盆地深部存在与大屯火山群深部相通的岩浆体,岩浆体的冷却由南向北迁移     

大别造山带白马尖花岗岩体的钕，锶同位素地球化学研究

大别造山带白马尖花岗岩体属燕山期侵入岩，为中生代大别山区岩浆活动的产物，为碰撞后花岗岩，锶，钕，同位素数据及稀土元素数据表明，白马尖花岗岩体为壳幔混合型，1．2－1．7Ga的钕模式年龄为其源岩的平均地壳存留年龄，北大别花岗岩类岩石的物质来源并不一致。     

论祁雨沟式金矿

祁雨沟金矿是典型的爆破角砾岩型金矿。系统地论述了其成矿地质背景、矿床地质、地球化学特征、及其成因意义。根据围岩蚀变和矿物包裹体温度、成分的研究,确定了矿床形成的物理化学条件及其各阶段的演变;通过氧同位素研究证明了成矿溶液的来源由早期岩浆水转变为晚期大气降水;用硫、碳和铅同位素组成说明成矿物质的复杂来源。以板块构造理论为指导,建立了矿床的形成模式,并指出找矿方向。