甘肃白银厂矿田早中寒武世酸性火山岩成因及源区特征的地球化学制约

从白银厂矿田早中寒武世酸性火山岩的地球化学研究入手，对其成因和源区特征进行了比较深入的探讨，认为本区酸性火山岩的源岩应是玄武岩和含水辉长质岩石的部分熔融形成的安山岩，源岩安山岩部分熔融形成该区流纹岩，而英安岩主要由流纹岩浆或与玄武岩浆混合或发生不明显的分离结晶形成．早-中寒武世，该区酸性火山岩的成岩环境为火山弧环境，当洋壳俯冲进入深处时，由于俯冲板片的脱水导致上地幔楔部分熔融形成源岩玄武岩，同时富水的流体萃取洋壳中的大离子亲石元素、轻稀土元素向上进入楔形地幔，使地幔橄榄岩富集大离子亲石元素．地幔中流体的增加导致下地壳中辉长质岩石的部分熔融形成了该区流纹岩的源岩--安山岩．熔融地幔底辟上升，由于高热流而引起下地壳局部熔融和混染，使该区酸性火山岩又具有陆壳混染的特征．     

镜泊湖全新世火山岩——岩浆的多样性

通过对镜泊湖全新世十余座火山的岩石化学及矿物化学研究表明,该火山岩属于一套富钾火山岩,包括粗面玄武岩、碧玄岩和响岩质碱玄岩三种不同的火山岩类型,这些小区域短时间内形成的多样性岩浆为来自不同程度钾质交代地幔的部分熔融.作者认为这些岩浆的成因机制可能为镜泊湖地处太平洋板块俯冲的东亚大陆弧后扩张区,来自地幔契或消减的深俯冲板片脱水的钾质流体从而导致镜泊湖地区之下小区域内高度的地幔化学非均一性和岩浆的多样性.根据普通辉石巨晶形成压力估计,响岩质碱玄岩岩浆在约52-54 km深处发生高压分离结晶作用.     

俯冲和岩浆过程中的地球深部碳循环

地球表层短周期的地表碳循环影响全球气候变化和地球宜居环境，而地球上90%以上的碳存在于地球内部，地球内部长周期的深部碳循环对地表碳循环产生重要影响。介绍了汇聚板块边界、离散板块边界、板块内部和新型海山等不同构造背景深部碳循环的研究现状，并阐述将来需要深入研究的科学问题，包括俯冲带脱碳机制及其效率、碳在地幔中的存在形式等。     

大同旧高山火山岩岩石学特征及构造意义

为了厘定山西大同旧高山火山岩的时代归属,探讨旧高山火山岩形成的构造环境及其构造背景,笔者对旧高山火山岩进行了野外地质调查、岩矿鉴定和主、微量元素地球化学特征研究,认为旧高山火山岩形成于早白垩世,为一套高钾钙碱性系列的中基性火山岩,火山作用以宁静式喷发为主;火山岩形成于大陆板内裂谷大地构造环境,岩浆来源于地幔与下地壳物质部分熔融的混合;火山岩的形成受控于晚中生代古太平洋板块向欧亚大陆俯冲的动力学背景。本结果对研究华北克拉通西北部的破坏具有重要意义。     

延边杜荒岭铜金矿区中酸性火成岩的地球化学特征及成岩机理

杜荒岭铜金矿是延边地区重要的浅成热液高硫化型矿床。对矿区内与成矿关系密切的中酸性岩石花岗闪长斑岩、石英闪长岩、花岗斑岩、花岗闪长岩进行主、微量地球化学研究。研究结果表明石英闪长岩、花岗闪长斑岩是俯冲板片提供的流体及熔体交代下地壳而形成的富集地幔源岩浆部分熔融的产物;花岗斑岩、花岗闪长岩是有俯冲沉积物贡献的俯冲洋壳部分熔融形成的埃达克质岩浆,在其上升过程中与俯冲板片提供的流体交代下地壳而形成的富集地幔源岩浆混合后派生的产物。具有埃达克质成因的花岗斑岩、花岗闪长岩是杜荒岭铜金矿床的成矿母岩。     

论地幔柱构造与板块构造的矛盾性和相容性

为了揭示地幔柱构造与板块构造的内在关系,针对地幔柱独特的地球物理和地球化学特征,通过与板块构造的对比：阐明了两者虽然在许多方面存在着矛盾,但在诠释岩石圈的解体和俯冲带的演化过程中都发挥着重要的作用;拆沉的冷板片聚集产生了超级冷地幔柱,由此导致了超级热地幔柱,冷热两个超级地幔柱的活动又控制了板块的运动和发展,由此可见,地幔柱构造理论对板块构造理论起着重要的补充和拓展作用。     

南海成因：岩石圈破裂与俯冲带相互作用新认识

 南海深部计划与国际大洋钻探航次取得了一系列创新进展与重大突破：1）发现南海陆缘岩石圈减薄之初未出现地幔蛇纹岩出露，且岩浆迅速出现；2）新提出南海不是“小大西洋”，而是“板缘张裂”盆地，与经典的大西洋型“板内张裂”陆缘模式不同；3）揭示南海受到俯冲带的强烈控制，提出俯冲诱发地幔上涌并影响南海岩浆活动。     

大陆碰撞与超高压变质

近30年来固体地球科学研究最重要的进展之一是认识到低密度大陆地壳能够俯冲到大于80千米的地幔深部,形成含有柯石英和金刚石等特殊矿物的超高压变质岩。地球     

房山岩体的岩浆来源、形成机制及动力学意义

房山岩体是华北东部典型的燕山期中酸性侵入杂岩体,其地球化学特征为富Si、Na、Al、Sr,亏损高场强元素(Nb、Ta),轻重稀土分异强烈,Sr-Nd同位素具有类似EMI型富集地幔的特点,表明其岩浆来自于加厚下地壳的部分熔融,并且中生代华北东部下地壳已经被早先的富集岩石圈地幔置换.不同基性程度岩浆的不完全混合是形成微粒闪长质包体的原因.侵入杂岩的角闪石压力计显示下地壳部分熔融形成的中酸性岩浆先后在19~8 km里的深度范围内结晶就位.古太平洋板块在地幔过渡带深度于早白垩世水平俯冲至太行山一线,洋壳脱水导致上覆地幔部分熔融,后者成为加热下地壳部分熔融的热源.     

汤加-克马德克俯冲带的地质构造与地震火山特征

2022年1月15日西南太平洋的洪阿哈阿帕伊岛海底火山发生了爆炸式的剧烈喷发，吸引了全球的关注。洪阿哈阿帕伊岛海底火山位于汤加-克马德克俯冲带，综合前期研究结果，对汤加-克马德克俯冲带的地质构造特征、地震和火山分布进行初步分析，发现：（1）从汤加-克马德克俯冲带弧前向海方向直到俯冲的太平洋板块，构造上主要表现为大规模正断层。（2）路易斯维尔海山链的俯冲将汤加-克马德克俯冲带分为北部的汤加俯冲带和南部的克马德克俯冲带，沿汤加俯冲带板块汇聚率为67～84 mm/a，沿克马德克俯冲带板块汇聚率为41～58 mm/a，板块俯冲速度的差异造成汤加俯冲带和克马德克俯冲带目前俯冲深度的不同。（3）在路易斯维尔海山链以北，太平洋板块上覆沉积物厚度不足0.4 km，而在南侧达到1 km左右，由于俯冲板块上覆沉积物厚度的差异而造成北部的汤加俯冲带和南部的克马德克俯冲带孕育地震能力的差异。这些认识对研究该俯冲带的火山喷发机制、大地震成因机理及其灾害风险具有重要意义。     

Holocene volcanic rocks in Jingbo Lake region ? Diversity of magmatism

During the time from 5500 a to 5200 a BP more than 10 Holocene volcanoes in Jingbo Lake region erupted and the volcanic rocks covered an area of about 500 km2. Holocene volcanic rocks in Jingbo Lake region belong to the potassium?rich rocks and contain three rock types: trachybasalts, basanites and phonotephrites. Various types of magmatism formed in a small area and in a short period of time came from partial melting of potassically?metasomatised lithospheric mantle. The diversity of magmatism can be explained by that Jingbo Lake is situated in the back?arc extensional region of East Asian continent subducted by the Pacific Ocean, and potassic fluid derived from mantle wedge or dehydration of subducted slab can result in a high heterogeneity of the mantle beneath this region. Based on the pressure estimation of clinopyroxene megacrysts, we estimate that phonotephrite magma fractionally crystallize at ca. 52?54 km down the earth.     

Magmatic and amagmatic seafloor generation at the ultraslow-spreading Gakkel ridge,Arctic Ocean

A high-resolution mapping and sampling study of the Gakkel ridge was accomplished during an international ice-breaker expedition to the high Arctic and North Pole in summer 2001. For this slowest-spreading endmember of the global mid-ocean-ridge system, predictions were that magmatism should progressively diminish as the spreading rate decreases along the ridge, and that hydrothermal activity should be rare. Instead, it was found that magmatic variations are irregular, and that hydrothermal activity is abundant. A 300-kilometre-long central amagmatic zone, where mantle peridotites are emplaced directly in the ridge axis, lies between abundant, continuous volcanism in the west, and large, widely spaced volcanic centres in the east. These observations demonstrate that the extent of mantle melting is not a simple function of spreading rate: mantle temperatures at depth or mantle chemistry (or both) must vary significantly along-axis. Highly punctuated volcanism in the absence of ridge offsets suggests that first-order ridge segmentation is controlled by mantle processes of melting and melt segregation. The strong focusing of magmatic activity coupled with faulting may account for the unexpectedly high levels of hydrothermal activity observed.     

Solid-liquid iron partitioning in Earth's deep mantle

Melting processes in the deep mantle have important implications for the origin of the deep-derived plumes believed to feed hotspot volcanoes such as those in Hawaii. They also provide insight into how the mantle has evolved, geochemically and dynamically, since the formation of Earth. Melt production in the shallow mantle is quite well understood, but deeper melting near the core-mantle boundary remains controversial. Modelling the dynamic behaviour of deep, partially molten mantle requires knowledge of the density contrast between solid and melt fractions. Although both positive and negative melt buoyancies can produce major chemical segregation between different geochemical reservoirs, each type of buoyancy yields drastically different geodynamical models. Ascent or descent of liquids in a partially molten deep mantle should contribute to surface volcanism or production of a deep magma ocean, respectively. We investigated phase relations in a partially molten chondritic-type material under deep-mantle conditions. Here we show that the iron partition coefficient between aluminium-bearing (Mg,Fe)SiO(3) perovskite and liquid is between 0.45 and 0.6, so iron is not as incompatible with deep-mantle minerals as has been reported previously. Calculated solid and melt density contrasts suggest that melt generated at the core-mantle boundary should be buoyant, and hence should segregate upwards. In the framework of the magma oceans induced by large meteoritic impacts on early Earth, our results imply that the magma crystallization should push the liquids towards the surface and form a deep solid residue depleted in incompatible elements.     

The chemical structure of the Hawaiian mantle plume

The Hawaiian-Emperor volcanic island and seamount chain is usually attributed to a hot mantle plume, located beneath the Pacific lithosphere, that delivers material sourced from deep in the mantle to the surface. The shield volcanoes of the Hawaiian islands are distributed in two curvilinear, parallel trends (termed 'Kea' and 'Loa'), whose rocks are characterized by general geochemical differences. This has led to the proposition that Hawaiian volcanoes sample compositionally distinct, concentrically zoned, regions of the underlying mantle plume. Melt inclusions, or samples of local magma 'frozen' in olivine phenocrysts during crystallization, may record complexities of mantle sources, thereby providing better insight into the chemical structure of plumes. Here we report the discovery of both Kea- and Loa-like major and trace element compositions in olivine-hosted melt inclusions in individual, shield-stage Hawaiian volcanoes--even within single rock samples. We infer from these data that one mantle source component may dominate a single lava flow, but that the two mantle source components are consistently represented to some extent in all lavas, regardless of the specific geographic location of the volcano. We therefore suggest that the Hawaiian mantle plume is unlikely to be compositionally concentrically zoned. Instead, the observed chemical variation is probably controlled by the thermal structure of the plume.     

The crust and mantle of Mars.

Clues to the history of Mars are recorded in the chemistry and structure of the planet's crust and mantle. The mantle is the rocky, interior region of the planet that transports heat generated during accretion and subsequent core formation. The crust formed by melting of the upper mantle, and has been shaped and re-distributed by impact, volcanism, mantle flow and erosion. Observations point to a dynamically active interior in the early phases of martian history, followed by a rapid fall-off in heat transport that significantly influenced the geological, geophysical and geochemical evolution of the planet, including the history of water and climate.     

Petrology and thermal structure of the Hawaiian plume from Mauna Kea volcano

There is uncertainty about whether the abundant tholeiitic lavas on Hawaii are the product of melt from peridotite or pyroxenite/eclogite rocks. Using a parameterization of melting experiments on peridotite with glass analyses from the Hawaii Scientific Deep Project 2 on Mauna Kea volcano, I show here that a small population of the core samples had fractionated from a peridotite-source primary magma. Most lavas, however, differentiated from magmas that were too deficient in CaO and enriched in NiO (ref. 2) to have formed from a peridotite source. For these, experiments indicate that they were produced by the melting of garnet pyroxenite, a lithology that had formed in a second stage by reaction of peridotite with partial melts of subducted oceanic crust. Samples in the Hawaiian core are therefore consistent with previous suggestions that pyroxenite occurs in a host peridotite, and both contribute to melt production. Primary magma compositions vary down the drill core, and these reveal evidence for temperature variations within the underlying mantle plume. Mauna Kea magmatism is represented in other Hawaiian volcanoes, and provides a key for a general understanding of melt production in lithologically heterogeneous mantle.     

Archaean ultra-depleted komatiites formed by hydrous melting of cratonic mantle

Komatiites are ultramafic volcanic rocks containing more than 18 per cent MgO (ref. 1) that erupted mainly in the Archaean era (more than 2.5 gigayears ago). Although such compositions occur in later periods of Earth history (for example, the Cretaceous komatiites of Gorgona Island), the more recent examples tend to have lower MgO content than their Archaean equivalents. Komatiites are also characterized by their low incompatible-element content, which is most consistent with their generation by high degrees of partial melting (30-50 per cent). Current models for komatiite genesis include the melting of rock at great depth in plumes of hot, diapirically rising mantle or the melting of relatively shallow mantle rocks at less extreme, but still high, temperatures caused by fluxing with water. Here we report a suite of ultramafic lava flows from the Commondale greenstone belt, in the southern part of the Kaapvaal Craton, which represents a previously unrecognized type of komatiite with exceptionally high forsterite content of its igneous olivines, low TiO(2)/Al(2)O(3) ratio, high silica content, extreme depletion in rare-earth elements and low Re/Os ratio. We suggest a model for their formation in which a garnet-enriched residue left by earlier cratonic volcanism was melted by hydration from a subducting slab.     

Arc-parallel flow in the mantle wedge beneath Costa Rica and Nicaragua

Resolving flow geometry in the mantle wedge is central to understanding the thermal and chemical structure of subduction zones, subducting plate dehydration, and melting that leads to arc volcanism, which can threaten large populations and alter climate through gas and particle emission. Here we show that isotope geochemistry and seismic velocity anisotropy provide strong evidence for trench-parallel flow in the mantle wedge beneath Costa Rica and Nicaragua. This finding contradicts classical models, which predict trench-normal flow owing to the overlying wedge mantle being dragged downwards by the subducting plate. The isotopic signature of central Costa Rican volcanic rocks is not consistent with its derivation from the mantle wedge or eroded fore-arc complexes but instead from seamounts of the Galapagos hotspot track on the subducting Cocos plate. This isotopic signature decreases continuously from central Costa Rica to northwestern Nicaragua. As the age of the isotopic signature beneath Costa Rica can be constrained and its transport distance is known, minimum northwestward flow rates can be estimated (63-190 mm yr(-1)) and are comparable to the magnitude of subducting Cocos plate motion (approximately 85 mm yr(-1)). Trench-parallel flow needs to be taken into account in models evaluating thermal and chemical structure and melt generation in subduction zones.     

Increased subaerial volcanism and the rise of atmospheric oxygen 2.5 billion years ago

The hypothesis that the establishment of a permanently oxygenated atmosphere at the Archaean-Proterozoic transition (approximately 2.5 billion years ago) occurred when oxygen-producing cyanobacteria evolved is contradicted by biomarker evidence for their presence in rocks 200 million years older. To sustain vanishingly low oxygen levels despite near-modern rates of oxygen production from approximately 2.7-2.5 billion years ago thus requires that oxygen sinks must have been much larger than they are now. Here we propose that the rise of atmospheric oxygen occurred because the predominant sink for oxygen in the Archaean era-enhanced submarine volcanism-was abruptly and permanently diminished during the Archaean-Proterozoic transition. Observations are consistent with the corollary that subaerial volcanism only became widespread after a major tectonic episode of continental stabilization at the beginning of the Proterozoic. Submarine volcanoes are more reducing than subaerial volcanoes, so a shift from predominantly submarine to a mix of subaerial and submarine volcanism more similar to that observed today would have reduced the overall sink for oxygen and led to the rise of atmospheric oxygen.     

Low electrical resistivity associated with plunging of the Nazca flat slab beneath Argentina

Beneath much of the Andes, oceanic lithosphere descends eastward into the mantle at an angle of about 30 degrees (ref. 1). A partially molten region is thought to form in a wedge between this descending slab and the overlying continental lithosphere as volatiles given off by the slab lower the melting temperature of mantle material. This wedge is the ultimate source for magma erupted at the active volcanoes that characterize the Andean margin. But between 28 degrees and 33 degrees S the subducted Nazca plate appears to be anomalously buoyant, as it levels out at about 100 km depth and extends nearly horizontally under the continent. Above this 'flat slab', volcanic activity in the main Andean Cordillera terminated about 9 million years ago as the flattening slab presumably squeezed out the mantle wedge. But it is unknown where slab volatiles go once this happens, and why the flat slab finally rolls over to descend steeply into the mantle 600 km further eastward. Here we present results from a magnetotelluric profile in central Argentina, from which we infer enhanced electrical conductivity along the eastern side of the plunging slab, indicative of the presence of partial melt. This conductivity structure may imply that partial melting occurs to at least 250 km and perhaps to more than 400 km depth, or that melt is supplied from the 410 km discontinuity, consistent with the transition-zone 'water-filter' model of Bercovici and Karato.