Roles for fluid and/or melt advection in forming high-P mafic migmatites, Fiordland, New Zealand

A series of striking migmatitic structures occur in rectilinear networks through western Fiordland, New Zealand, involving, for the most part, narrow anorthositic dykes that cut hornblende‐bearing orthogneiss. Adjacent to the dykes, host rocks show patchy, spatially restricted recrystallization and dehydration on a decimetre‐scale to garnet granulite. Although there is general agreement that the migration of silicate melt has formed at least parts of the structures, there is disagreement on the role of silicate melt in dehydrating the host rock. A variety of causal processes have been inferred, including metasomatism due to the ingress of a carbonic, mantle‐derived fluid; hornblende‐breakdown leading to water release and limited partial melting of host rocks; and dehydration induced by volatile scavenging by a migrating silicate melt. Variability in dyke assemblage, together with the correlation between dehydration structures and host rock silica content, are inconsistent with macroscopic metasomatism, and best match open system behaviour involving volatile scavenging by a migrating trondhjemitic liquid.     

The anatomy of Continental Flood Basalt Provinces: geological constraints on the processes and products of flood volcanism

The internal architecture of the immense volumes of eruptive products in Continental Flood Basalt Provinces (CFBPs) provides vital clues, through the constraint of a chrono-stratigraphic framework, to the origins of major intraplate melting events. This work presents close examination of the internal facies architecture and structure, duration of volcanism, epeirogenetic uplift associated with CFBPs, and the potential environmental impacts of three intensely studied CFBPs (the Parana-Etendeka, Deccan Traps and North Atlantic Igneous Province). Such a combination of key volcanological, stratigraphic and chronologic observations can reveal how a CFBP is constructed spatially and temporally to provide crucial geological constraints regarding their development.

Using this approach, a typical model can be generated, on the basis of the three selected CFBPs, that describes three main phases of flood basalt volcanism. These phases are recognized in Phanerozoic CFBPs globally. At the inception of CFBP volcanism, relatively low-volume transitional-alkaline eruptions are forcibly erupted into exposed cratonic basement lithologies, sediments, and in some cases, water. Distribution of initial volcanism is strongly controlled by the arrangement of pre-existing topography, the presence of water bodies and local sedimentary systems, but is primarily controlled by existing lithospheric and crustal weaknesses and concurrent regional stress patterns. The main phase of volcanism is typically characterised by a culmination of repeated episodes of large volume tholeiitic flows that predominantly generate large tabular flows and flow fields from a number of spatially restricted eruption sites and fissures. These tabular flows build a thick lava flow stratigraphy in a relatively short period of time (c. 1–5 Ma). With the overall duration of flood volcanism lasting 5–10 Ma (the main phase accounting for less than half the overall eruptive time in each specific case). This main phase or ‘acme’ of volcanism accounts for much of the CFBP eruptive volume, indicating that eruption rates are extremely variable over the whole duration of the CFBP. During the waning phase of flood volcanism, the volume of eruptions rapidly decrease and more widely distributed localised centres of eruption begin to develop. These late-stage eruptions are commonly associated with increasing silica content and highly explosive eruptive products. Posteruptive modification is characterised by continued episodes of regional uplift, associated erosion, and often the persistence of a lower-volume mantle melting anomaly in the offshore parts of those CFBPs at volcanic rifted margins.     

玄武岩浆起源和演化的一些基本概念以及对中国东部中-新生代基性火山岩成因的新思路

以全球大地构造为背景讨论了玄武岩浆起源和演化的一些基本概念.这些概念的正确理解有助于合理解释各种环境中火成岩的形成机制,也有助于依据野外岩石组合来判别古构造环境.在此基础上结合已有资料和观察,对中国东部中生代岩石圈减薄及中-新生代基性火山岩成因提出了一些新解释.这些解释与地质观察相吻合,且符合基本的物理学原理.虽然中国东部基性火山活动可称为"板内"火山活动,但它实际上是板块构造的特殊产物.中国东部中生代岩石圈减薄是其下部被改造为软流层的缘故.这种改造是加水"软化"所致.水则源于中国东部地幔过渡带(410～660 km)内古太平洋(或其前身)俯冲板块脱水作用.其将岩石圈底部改造为软流层的过程,实际上就是岩石圈减薄的过程.因为软流层是地幔对流的重要部分,而大陆岩石圈则不直接参与地幔对流.中生代玄武岩具有εNd＜0的特征,说明其源于新近改造而成的软流层,亦即原古老岩石圈之底部.中国大陆北北东-南南西向的海拔梯度突变界线与东-西部重力异常,陆壳厚度变化,以及地幔地震波速变化梯度吻合.因此可将北北东-南南西向梯度线称为"东-西梯度界".该界东-西海拔高差(西部高原与东部丘陵平原),陆壳厚度差异(西部厚而东部薄)和100～150 km的深度范围地幔地震波速差异(西部快而东部慢),均受控于上地幔重力均衡原理.这表明西部高原岩石圈厚度＞150～200 km,而东部丘陵平原岩石圈厚度＜80km."遥远"的西太平洋俯冲带具有自然的地幔楔吸引作用.此吸引作用可引起中国东部"新生"软流层东流.软流层东流必将引起西部高原底部软流层的东向补给(流动).这一过程必然导致东移软流层的减压,即从西部的深源(岩石圈深度＞150～200 km处)到东部的浅源(岩石圈深度～80km处).东移软流层的减压分熔可合理解释具有软流圈地球化学特征(εNd＞0)的新生代中国东部基性火山活动及玄武岩的成因.这些对中国东部中-新生代地质过程的解释,将为更加细致的,以岩石学和地球化学为主的讨论所验证.     

拉萨地体内低速异常成因的探讨--壳内局部熔融的地震层析证据

青藏高原南部天然地震体波的层析反演图像描绘出拉萨地体内在15～90km深度内低速异常的分布特征。在研究速度结构的基础上，根据熔融程度与纵波波速呈倒数衰减的特性，论证了拉萨地体中低速体的出现与壳内的局部熔融有关。壳内局部熔融则来源于板块俯冲、地壳增厚产生的热而非幔源侵入所造成。同时，也发现了在拉萨以东中下地壳低速体有向东发展的趋势。大面积部分熔融层分布的深度范围约在15～35km处。另外，据藏南地区的SKS波分裂时间延迟很小的特点，推测藏南地幔中可能不存在各向异性，也就是没有足够的热源使各向异性矿物的品格重新定位。这从另一方面佐证了部分熔融仅存在于地壳内而不是地幔中。     

Origin of Exceptionally Abundant Phonolites on Ua Pou Island (Marquesas, French Polynesia): Partial Melting of Basanites Followed by Crustal Contamination

On the basis of the first systematic mapping of Ua Pou, longknown for its exceptionally abundant phonolites, we estimatethat these rocks cover 65% of the surface of the island whereasmafic lavas cover 27% and intermediate ones 8%. The silica-undersaturatedsuite was erupted in a restricted time span (2·9–2·35Myr), following the emplacement of tholeiites derived from ayoung HIMU-type source at c. 4 Ma. Primitive basanites, derivedfrom a heterogeneous mantle source with a dominant EM II + HIMUsignature, represent likely parental magmas. The series is characterizedby a Daly gap defined by a lack of phonotephrites. We considerthat the most likely model for the origin of evolved lavas ispartial melting at depth of primitive basanites, leaving anamphibole-rich residuum and producing tephriphonolitic magmas.These tephriphonolitic magmas may have evolved by closed-systemfractional crystallization towards Group A phonolites. Threeother groups of phonolites could have been derived from tephriphonoliticmagmas by open-system fractional crystallization processes,characterized respectively by seawater contamination (GroupB), assimilation of nepheline syenite-type materials (GroupC) and extreme fractionation coupled with assimilation of theunderlying oceanic crust (Group D). The prominence of evolvedlavas is a consequence of their origin from partial meltingof mafic precursors followed by crustal contamination. KEY WORDS: Marquesas; French Polynesia; phonolite; partial melting; contamination     

PEIV模型参数估计新算法

PEIV(Partial Errors-In-Variables)模型是EIV模型的扩展,它能解决系数矩阵含有非随机元素或存在结构特性的问题。针对常规PEIV模型算法的复杂性,提出了一种PEIV模型参数估计的新算法。该算法将系数矩阵含误差的元素看成是一类观测值,与平差模型原观测值构成两类观测值,将PEIV平差模型表示为类似于传统的最小二乘间接平差模型,再通过非线性最小二乘平差理论,推导出了算法的迭代公式和精度评定公式。算法迭代格式与间接平差类似,通过算例验证了算法的可行性和正确性。     

青藏高原拉萨地块西部念青唐古拉岩群的地球化学特征及构造意义

拉萨地块西部呈断块状沿狮泉河-申扎-嘉黎蛇绿混杂岩带附近分布的念青唐古拉岩群被认为是前寒武纪变质基底。本文对念青唐古拉岩群进行了系统的岩石学、地球化学、同位素年代学及构造地质学研究。研究结果表明片岩-片麻岩-变粒岩含十字石、石榴子石等特征变质矿物,遵循粒度分异规律,其原岩可能为来自冈瓦纳古陆核北缘中新元古代弧盆体系的活动大陆边缘浊积岩。斜长角闪岩具低硅、高铁镁、富钙的基性岩特征,其原岩为岛弧型基性火山岩。念青唐古拉岩群中的花岗伟晶岩锆石LA-ICPMS U-Pb年龄为1150±13Ma,具过铝质S型花岗岩地球化学特征,可能为中元古代(1150±13 Ma)以前就开始沉积的念青唐古拉岩群基底岩石通过部分熔融形成。与花岗伟晶岩渐变过渡接触的二云斜长片麻岩第一组变质重结晶锆石U-Pb年龄为701±15 Ma,结合十字石特征变质矿物,暗示了该地区中温高压变质作用的峰期变质,变质程度达角闪岩相;第二组热液流体锆石UPb年龄为301±8.4 Ma,可能与冈瓦纳大陆北缘古特提斯洋演化过程中的岩浆热液作用有关。     

岩石中的压力影形成的实验观测研究

野外地质观察发现,在大陆地壳变质岩中可以广泛观察到围绕一个大的单晶或者硬质点的两端区域填充低粘度相物质形成的压力影。为了定量研究岩石材料中压力影的形成条件,本文利用高精度Paterson气体介质变形装置,对含有刚性球的圣卡罗橄榄石和洋中脊玄武岩(MORB)的混合物圆柱型样品进行了高温高压扭转变形试验。变形实验前样品的初始熔融均匀分布,比例为φ≈0.05,变形试件尺寸为D8.9mm×L5.5mm,内含8粒直径约1mm的刚性球。扭转变形试验温度为1473K,围压为300MPa,应变率为γ≈1×10~(-4)s~(-1),最大剪切变形为γ≈4。实验结果表明,岩石受到扭转力的作用产生变形之后,当局部剪切应变达到γ≈1时,可以在刚性球周围形成熔融富集带和熔融贫乏带,即压力影构造,围绕刚性球对称分布。由于熔融分布的不均一性,富集带熔融比例上升,最高可以达到φ_(high)=0.1~0.3,熔融贫乏带熔融比例下降,含量为φ_(low)=0.01~0.02。由于刚性球对其周围的压力分布的扰动区域大约为刚性球的尺度范围,因此,在离开刚性球一定距离后,熔融趋于均匀分布。     

皖南晚中生代花岗闪长岩地球化学:成岩成矿制约

皖南地区是铜、钼、金多金属成矿区,成矿与晚中生代花岗闪长岩类关系密切。近十年来,皖南花岗闪长岩的成因仍然存在分歧。本次报道了皖南花岗闪长岩全岩主、微量元素和锆石原位元素数据。皖南花岗闪长岩(Si O2=64.3%~70.8%)为高钾钙碱性、过铝质岩石,具有相似的埃达克岩特征:高Si O2、Sr/Y(17.1)和(La/Yb)N(14.9)比值,低Yb(1.72×10-6)和Y(18.4×10-6)含量。它们也具有较低Al2O3和Cr(3.40×10-6~10.0×10-6)含量、低Mg#(0.34~0.42)和Nb/Ta(9.6~13.3)值,高K2O和Ba(404×10-6)含量,高K2O/Na2O(0.89~1.55)、Th/La(0.27~0.51)和Th/U(2.79~7.49)比值。锆石原位地球化学特征显示其岩浆源区为低温(锆石Ti-in-zircon温度均值674℃)和高氧逸度(lgfO2集中在-21.4~-9.18,均值-16.4;锆石Ce4+/Ce3+平均值276)的陆壳。这些特征说明皖南花岗闪长岩可能起源于较年轻的加厚下地壳的部分熔融,并经历了斜长石、钾长石和铁镁矿物等结晶分异作用。它们可能形成于与古太平洋板块俯冲密切相关的大陆活动边缘弧至弧后拉张构造转换背景。本区大规模Cu、Mo、Au成矿作用与岩浆的高氧逸度密切相关,而锆石Ce4+/Ce3+可作为矿床勘探一个有效的指标。     

从藏南陆-陆碰撞带深部结构构造演化探讨斑岩铜矿的成岩成矿问题

本文以INDEPTH项目对印度大陆与欧亚大陆碰撞带深部成像结果为基础,从构造演化角度探讨藏南陆-陆碰撞带冈底斯斑岩铜矿带的成矿作用问题。深部探测给出的碰撞带深部结构与侯增谦等地质学家提出的深部结构有较大的异同,如何协调起来以深化对藏南陆-陆碰撞条件下成矿作用的认识,这是本文讨论的中心。藏南碰撞带成矿实际上是在新特提斯大洋岩石圈俯冲形成的冈底斯岩浆弧成矿作用的基础上,再经过陆-陆碰撞挤压强烈改造后的再成矿。碰撞带的深部结构构造演化的特点是:(1)新特提斯大洋岩石圈板块向北连续俯冲了约120 Ma,形成的冈底斯陆缘火山岩浆弧带,这导致了陆缘带地壳增厚并含有大量的地幔岩浆流体物质(如南美安第斯成矿带那样);(2)在印度大陆与冈底斯陆缘弧接近碰撞时,在对挤中新特提斯大洋洋壳与大洋岩石圈地幔发生向上挤出与向下拆沉,并使部分洋壳残片和大洋岩石圈物质保存在中上地壳内;(3)两大陆岩石圈碰撞对接后,印度岩石圈地幔加深达70~80 km并沿地壳底部向北推进,并将加厚地壳内大量的成矿物质、钙碱性岩浆,洋壳及新生的下地壳,以及部分地幔物质从地壳底部将其围限起来,成为后期再成矿的物质基础;(4)查明了碰撞带深部壳/幔间产生了一层中间速度层(相当于MASH层),在中上地壳部位出现一层巨大的部分熔融层;(5)在碰撞挤压下冈底斯带内产生多组断裂构造,大型逆冲断裂系与背冲断裂,并引发了含矿岩浆的再活动,并在浮力(下地壳内)和挤压力作用下多次活动上升生成斑岩型铜矿床;(6)成矿后地表遭受过强烈的风化剥蚀作用,使矿床出露地表。