大同新生代火山岩浆的快速喷发——来自橄榄石地幔捕掳晶的证据

量化研究幔源岩浆从源区运移至喷发或者侵位的时间尺度，对理解基性岩浆作用具有重要意义。然而，对于岩浆的喷发和就位的时间尺度研究仍缺乏有效的约束，位于我国华北克拉通北部山西大同新生代火山岩群是理想的研究地区。本文以该火山群～0.2 Ma喷发的神泉寺碱性玄武岩为研究对象，重点研究其中携带的地幔橄榄石捕掳晶来约束喷发前的时间尺度。通过对其开展详细的矿物化学研究，发现地幔捕掳晶核部的Fo值高达97.7,为极富镁橄榄石，结合其极低的Ca、Mn和Ni含量特征，认为它们捕获自被交代的地幔橄榄岩。另外，地幔橄榄石捕掳晶发育明显的CaO成分环带，表明其在地壳岩浆系统内经历了复杂的岩浆演化过程。地幔橄榄石捕掳晶反应边宽度变化很大，说明它们在源区被捕获时及在运移过程中经过了多次破碎过程。橄榄石捕掳晶最边缘的Fo值为70左右，平衡计算表明它们在边部已与主岩浆(碱性玄武岩)达到平衡。Fe-Mg元素扩散计时结果显示，橄榄石地幔捕掳晶仅在岩浆中滞留了几个月的时间。对于40～70 km的岩石圈地幔厚度来说，岩浆平均上升速率最快可能超过500 m/d。     

不同应力路径下剪切带的数值模拟

采用回映应力更新算法,编写了基于伏斯列夫面的超固结黏土本构关系模型子程序,嵌入非线性有限元软件ABAQUS。通过对单元试验进行三轴压缩、三轴伸长及平面应变等问题的模型预测,再现了超固结黏土在不同初始超固结比和应力路径时的变形和强度特性,从而验证了子程序的正确性。借助该本构模型,对三轴压缩、三轴伸长及平面应变应力路径下超固结黏土体变形局部化问题,进行了三维数值模拟。分析结果表明：超固结黏土在三轴压缩及伸长状态时,土体变形局部化在应力-应变关系软化时出现,而平面应变状态时,在应力-应变关系硬化阶段出现,其超固结黏土的剪胀特性在剪切带的形成过程中起重要作用。     

Rates of magma ascent and depths of magma reservoirs beneath La Palma (Canary Islands)

Peridotitic mantle xenoliths from historic and prehistoric eruptions on La Palma show many similarities. Prolonged reactions of the xenoliths with their host magmas have been used to place constraints on the magma transport system beneath the island. All xenoliths show crystalline selvages and 0.9–2.6 mm wide diffusion zones in olivine along most of their surface. Diffusion kinetics in olivine, combined with fluid inclusion barometry, document that selvages and diffusion zones formed at crustal levels within 8 to about 100 years. Some xenolith fractures lack selvages and were in contact with the host magma for less than 4 days. A multistage magma ascent is proposed: (i) peridotite wall rock was fragmented and became incorporated into the ascending magma years to decades prior to the eruption; (ii) the xenoliths were rapidly transported to, and deposited in, crustal magma reservoirs, forming selvages and diffusion zones at the xenolith rims; (iii) renewed fragmentation of the xenoliths occurred days to hours prior to eruption, possibly by decompressive strain fracturing during rapid ascent.     

Effects of magma storage and ascent on the kinetics of crystal growth

The size distributions of crystals of olivine, plagioclase and oxides of the 1991/93 eruption at Mt. Etna (Italy) are analyzed. The simultaneous collection of this information for different minerals gives precious insight into the cooling history of lavas. Three distinct episodes are detectable: a storage of the magma in a deep reservoir, characterized by nearly constant and low nucleation and growth rates (near to equilibrium); an ascent phase, with an ever increasing nucleation rate related to volatile exsolution; and finally a quenching phase. In addition to geochemical and geophysical evidence, the similarity of the crystal size distributions of the present eruption with those of previous ones of this century makes it possible to exclude that crystal size distributions of Etnean lavas are due to mixing of different populations. This strongly suggests that the main features of the volcano feeding system have not changed despite observed variations in the magma output rates.     

The dynamics of magma-mixing during flow in volcanic conduits

The production of mixed magmas (streaky pumice) during flow in a volcanic conduit has been modelled in the laboratory by studying the flow of two miscible fluids of differing viscosity passing concentrically through a vertical pipe. In the experiments reported in this paper, the outermost fluid is the more viscous, as would be the case when two magmas are simultaneously tapped from a zoned chamber in which silicic magma overlies mafic magma. At a Reynolds number (Re) which is much less than that required for turbulence in isoviscous pipe flow, the interface between two liquids of different viscosity can become unstable. Growth of the instability and mixing proceed when Re, based on the properties of the inner, less viscous fluid (Re _i), is greater than approximately 3 if between 10% and 90% of the flowing fluid is composed of the more viscous fluid. Outside this range of flow rate ratios, higher Re _i and viscosity ratios are required to ensure mixing. When the viscosity ratio U10 the unstable flow takes the form of an asymmetric, sinusoidal wave and at higher viscosity ratios axisymmetric, bead-like waves are the dominant instability. Entrainment across the boundaries of these wavy interfaces results in the production of streaky mixtures of the two liquids. The degree of mixing increases with Re ₁, U and distance downstream. Application of experimental results to magmatic situations shows that mixing will be possible in eruptions which tap layers of different viscosity from a stratified chamber. If a volcanic feeder is allowed to become lined by silicic magma before a mafic magma layer is drawn up from the chamber then a mixed pumice (or lava) sequence will ensue. Alternatively, if draw-up occurs when the feeder is still propagating away from the chamber, the slower flowing silicic magma may be overtaken by the faster flowing mafic magma. The advancing conduit will then have mafic or hybrid chilled margins enclosing a silicic interior, i.e. the usual arrangement in composite dykes and sills. Simultaneous tapping of silicic and underlying mafic magmas from a chamber can thus lead to magma mixing and to the emplacement of either mixed pumice sequences or composite intrusions, depending on the history of magma withdrawal and the dynamics of flow in the conduit.     

Generation of CO2-rich melts during basalt magma ascent and degassing

To test mechanisms of basaltic magma degassing, continuous decompressions of volatile-bearing (2.7–3.8 wt% H₂O, 600–1,300 ppm CO₂) Stromboli melts were performed from 250–200 to 50–25 MPa at 1,180–1,140 °C. Ascent rates were varied from 0.25 to ~1.5 m/s. Glasses after decompression show a wide range of textures, from totally bubble-free to bubble-rich, the latter with bubble number densities from 10⁴ to 10⁶ cm^?3, similar to Stromboli pumices. Vesicularities range from 0 to ~20 vol%. Final melt H₂O concentrations are homogeneous and always close to solubilities. In contrast, the rate of vesiculation controls the final melt CO₂ concentration. High vesicularity charges have glass CO₂ concentrations that follow theoretical equilibrium degassing paths, whereas glasses from low vesicularity charges show marked deviations from equilibrium, with CO₂ concentrations up to one order of magnitude higher than solubilities. FTIR profiles and maps reveal glass CO₂ concentration gradients near the gas–melt interface. Our results stress the importance of bubble nucleation and growth, and of volatile diffusivities, for basaltic melt degassing. Two characteristic distances, the gas interface distance (distance either between bubbles or to gas–melt interfaces) and the volatile diffusion distance, control the degassing process. Melts containing numerous and large bubbles have gas interface distances shorter than volatile diffusion distances, and degassing proceeds by equilibrium partitioning of CO₂ and H₂O between melt and gas bubbles. For melts where either bubble nucleation is inhibited or bubble growth is limited, gas interface distances are longer than volatile diffusion distances. Degassing proceeds by diffusive volatile transfer at the gas–melt interface and is kinetically limited by the diffusivities of volatiles in the melt. Our experiments show that CO₂-oversaturated melts can be generated as a result of magma decompression. They provide a new explanation for the occurrence of CO₂-rich natural basaltic glasses and open new perspectives for understanding explosive basaltic volcanism.     

On the ascent and emplacement of granitoid magma bodies dynamic-thermal numerical models

The intrusion of granitoid magmas is understood as a lower and mid crustal process. Field observations and laboratory experiments give strong reason that most granitoid plutons are formed by diapiric ascent and emplacement of large magma bodies.On this basis, the ascent and emplacement of granitoid magmas is modelled by two-dimensional finite element calculations. The physical concept for this process provides convective transport of matter and heat, an isolated finite source region, variable source temperatures as well as variable density and viscosity contrasts.The model calculations show that the structural development of the model intrusion bodies is highly dependent on the physical properties of the magma and its surroundings. The most important among them are density and viscosity. Due to the different initial conditions, stocks of several plutons in the case of high viscosity contrast or flat magma sources as well as nappe-shaped intrusion structures as a result of low viscosity contrast can be understood by the intrusive mode of emplacement. The enlargement of the negative density contrast leads to an increase of the rate of ascent, so that more advanced intrusion structures are developed.

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Zusammenfassung Die Intrusion granitoider Magmen ist ein Prozeß der unteren und mittleren Kruste. Feldbefunde und Laboruntersuchungen geben Hinweise darauf, daß die meisten granitoiden Plutone durch diapirischen Aufstieg und Platznahme ausgedehnter Magmenkörper entstehen.Auf dieser Grundlage werden der Aufstieg und die Platznahme granitoider Magmen mit Hilfe von zweidimensionalen Finite Elemente Rechnungen modelliert. Das physikalische Konzept beinhaltet den konvektiven Transport von Masse und Energie, eine isolierte finite Quellregion, veränderliche Quelltemperaturen sowie einen variablen Dichte- und Viskositätskontrast.Die Modellrechnungen zeigen, daß die strukturelle Entwicklung der Modellmagmenkörper in hohem Maße von den physikalischen Parametern des Magmas und seiner Umgebung, vor allem Dichte und Viskosität, abhängt. Gemäß den unterschiedlichen Anfangsbedingungen können sowohl einige stockförmige Plutone im Falle eines hohen Viskositätskontrastes oder flacher Magmaquellen als auch deckenförmige Intrusionsstrukturen als Folge eines geringen Viskositätskontrastes mit Hilfe des intrusiven Einlagerungskonzeptes verstanden werden. Die Erhöhung des negativen Dichtekontrastes führt zu einer Erhöhung der Aufstiegsrate, so daß fortgeschrittenere Platznahmestrukturen erreicht werden können.

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Résumé L'intrusion des magmas granitoïdes est un processus qui intéresse la croûte inférieure et moyenne. Les observations de terrain et les expériences en laboratoire fournissent des arguments très sérieux en faveur de la formation des plutons par montée diapirique et mise en place de corps magmatiques de grandes dimensions.Sur base de cette conception, la montée et la mise en place de magmas granitoïdes a fait l'objet d'une modélisation par éléments finis à deux dimensions. Un tel modèle fait appel à un transport convectif de matière et de chaleur, à une région-source isolée de dimension finie, à une source de température variable ainsi qu' à divers contrastes de densité et de viscosité.Les calculs montrent que le développement structural des corps intrusifs ainsi modélisés dépend essentiellement des propriétés physiques du magma et de son encaissant, en particulier de la densité et de la viscosité. Etant données diverses conditions initiales, la modélisation rend compte de plusieurs types de culots plutoniques dans le cas de contrastes de viscosité élevés ou de sources de magma d'extension horizontale, ainsi que d'intrusions en forme de nappe dans le cas de faibles contrastes de viscosité. L'accroissement des contrastes de viscosité négatifs contribue à augmenter la vitesse d'ascension, ce qui permet le développement de structures d'intrusion plus évoluées.

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Notation a thermal expansion coefficient - C_p specific heat capacity - Di dissipation number (model specific) - g gravity acceleration - dynamic viscosity - h heigth of model - thermal diffusivity - Q heat flow - Ra Rayleigh number - R(v) differential operator - p density - t time - T absolute temperature - v velocity - V volume - w vertical component of velocity - x horizontal coordinate - stream function - z vertical coordinate     

Adiabatic temperature changes of magma–gas mixtures during ascent and eruption

Most quantitative studies of flow dynamics in eruptive conduits during volcanic eruptions use a simplified energy equation that ignores either temperature changes, or the thermal effects of gas exsolution. In this paper we assess the effects of those simplifications by analyzing the influence of equilibrium gas exsolution and expansion on final temperatures, velocities, and liquid viscosities of magma-gas mixtures during adiabatic decompression. For a given initial pressure (p₁), temperature (T₁) and melt composition, the final temperature (T_f) and velocity (u_max) will vary depending on the degree to which friction and other irreversible processes reduce mechanical energy within the conduit. The final conditions range between two thermodynamic end members: (1) constant enthalpy (dh=0), in which T_f is maximal and no energy goes into lifting or acceleration; and (2) constant entropy (ds=0), in which T_f is minimal and maximum energy goes into lifting and acceleration. For ds=0, T₁=900 °C and p₁=200 MPa, a water-saturated albitic melt cools by ~200 °C during decompression, but only about 250 °C of this temperature decrease can be attributed to the energy of gas exsolution per se: the remainder results from expansion of gas that has already exsolved. For the same T₁ and p₁, and dh=0, T_f is 10-15 °C hotter than T₁ but is about 10-25 °C cooler than T_f in similar calculations that ignore the energy of gas exsolution. For ds=0, p₁=200 MPa and T₁=9,000 °C, assuming that all the enthalpy change of decompression goes into kinetic energy, a water-saturated albitic mixture can theoretically accelerate to ~800 m/s. Similar calculations that ignore gas exsolution (but take into account gas expansion) give velocities about 10-15% higher. For the same T₁, p_I=200 MPa, and ds=0, the cooling associated with gas expansion and exsolution increases final melt viscosity more than 2.5 orders of magnitude. For dh=0, isenthalpic heating decreases final melt viscosity by about 0.7 orders of magnitude. Thermal effects of gas exsolution are responsible for less than 10% of these viscosity changes. Isenthalpic heating could significantly reduce flow resistance in eruptive conduits if heat generation were concentrated along conduit walls, where shearing is greatest. Isentropic cooling could enhance clast fragmentation in near-surface vents in cases where extremely rapid pressure drops reduce gas temperatures and chill the margins of expanding pyroclasts.     

Multi-stage magma ascent beneath the Canary Islands: evidence from fluid inclusions

Gabbroic and ultramafic xenoliths and olivine and clinopyroxene phenocrysts in basaltic rocks from Gran Canaria, La Palma, El Hierro, Lanzarote and La Gomera (Canary Islands) contain abundant CO₂-dominated fluid inclusions. Inclusion densities are strikingly similar on a regional scale. Histogram maxima correspond to one or more of the following pressures: (1) minimum 0.55 to 1.0 GPa (within the upper mantle); (2) between 0.2 and 0.4 GPa (the Moho or the lower crust); (3) at about 0.1 GPa (upper crust). Fluid inclusions in several rocks show a bimodal density distribution, the lower-density maximum comprising both texturally early and late inclusions. This is taken as evidence for an incomplete resetting of inclusion densities, and simultaneous formation of young inclusions, at well-defined magma stagnation levels. For Gran Canaria, pressure estimates for early inclusions in harzburgite and dunite xenoliths and olivine phenocrysts in the host basanites overlap at 0.9 to 1.0 GPa, indicating that such magma reservoir depths coincide with levels of xenolith entrainment into the magmas. Magma chamber pressures within the mantle, inferred to represent levels of mantle xenolith entrainment, are 0.65–0.95 GPa for El Hierro, 0.60–0.68 GPa for La Palma, and 0.55–0.75 GPa for Lanzarote. The highest-density fluid inclusions in many Canary Island mantle xenoliths have probably survived in-situ near-isobaric heating at the depth of xenolith entrainment. Inclusion data from all islands indicate ponding of basaltic magmas at Moho or lower crustal depths, and possibly at an additional higher level, strongly suggestive of two main crustal accumulation levels beneath each island. We emphasize that repeated magmatic underplating of primitive magmas, and therefore intrusive accretion, are important growth mechanisms for the Canary Islands, and by analogy, for other ocean islands. Comparable fluid inclusion data from primitive rocks in other tectonic settings, including Iceland, Etna and continental rift systems (Hungary, South Norway), indicate that magma accumulation close to Moho depths shortly before eruption is not, however, restricted to oceanic intraplate volcanoes. Lower crustal ponding and crystallization prior to eruption may be the rule rather than the exception, independent of the tectonic setting. Received: 30 May 1997 / Accepted: 6 February 1998     

Numerical simulations of ice accumulation under ice cover along a river bend

In this paper, the k-? two-equation turbulence model has been used to simulate ice accumulation under ice cover along a river bend. A 2D depth-averaged numerical model has been developed in a nonorthogonal coordinate system with nonstaggered curvilinear grids. In this model, the contravariant velocity has been treated as an independent variable. To avoid the pressure oscillation in the nonstaggered grids, the momentum interpolation has been introduced to interpolate variables at the interface. The discretization equations have been solved by using pressure correction algorithms. An equation has been developed for describing the deformation of ice jam bottom. The thickness distribution of ice accumulation (ice jam) along the bend has been simulated. The developed model has been applied to the experimental studies under different conditions carried out at the Hefei University of Technology. Results indicate that all simulated thickness of ice accumulation agrees reasonably well with the measured thickness of ice accumulation in laboratory.     

Morphometric analysis of magmatic enclaves: a tool for understanding magma vesiculation and ascent

The extent of deformation of magmatic enclaves that occur in different portions of the Khaggiar endogenous lava dome (Island of Pantelleria, Italy) has been quantified using two morphometric techniques: thin-plate splines and fractals. Deformation of enclaves decreases from the outer portions of the dome to the more internal portions, defining two exponential trends. The amount and distribution of vesicles have also been quantified using image analysis of digital images obtained by a scanning electron microscope. The variation of deformation of enclaves correlates with the variation of their vesicle content, suggesting that deformation and vesiculation are related. We envisaged a continuous feedback system between vesiculation of enclaves and radial forces exerted by the surrounding host magma during the growth of the dome. These relationships are used as dynamic markers to infer the eruptive style of the endogenous dome. In particular, it is suggested that the variation of vesicularity of enclaves is related to the pressure exerted by magma on the extrusion vent. This resulted in enclaves being more vesicular and more deformed in the outer portions of the dome that emplaced first and at lower pressure, and less vesicular and less deformed in the more internal portions that emplaced later and at higher pressure. We interpret the occurrence of the two trends in the variation of deformation and porosity as related to two main eruptive pulses of dome growth.     

Granite magma migration and emplacement along thrusts

This paper investigates the influence exerted by brittle tectonic structures in the emplacement of granite plutons in contractional settings. We address both cases where contractional tectonics and magma intrusion are (1) coeval, to study how active contractional tectonics controls the transport of magma, and (2) diachronous, to study the role of pre-existing structures on the transport of magma. In light of new experimental models, we show that magma can rise along thrusts ramps and flats. This phenomenon occurs for both low-viscosity magma (basalts to andesite) and high-viscosity magma (dry granite). The experimental results also allow the evaluation of the role played by magma viscosity in determining pluton geometries. In addition, a review of literature demonstrates a spatial and causal relationship between granites and thrusts and highlights the geometric control of magma pathways in the pluton final shape. The abundance of subhorizontal and tabular granitic intrusions indicates that the location of inflating granitic sills along thrust flats can be common. We argue that active and pre-existing flats-and-ramps thrusts provide a preferential continuous planar anisotropy susceptible to become a granitic magma migration pathway.     

On the character of magma differentiation in a volcanic vent

The lavas of the Kljuchevsky volcano which effused first and from higher horizons of the volcano, were somewhat more acid as compared to the following lava flows. Simultaneously, changes occurred in the composition of the minerals of the lavas. Their olivine and pyroxenes correspondingly changed from more ferruginous to less ferruginous, and the plagioclases changed from less basic to more basic. These changes of the composition of the minerals in the lavas were, by the author's supposition, the result of a differentiation due to temperature-diffusion.

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Zusammenfassung Die Laven des Vulkans Klyutschewsky, die als erste ausgeflossen sind und aus einem höheren Stockwerk stammen, sind etwas saurer im Vergleich zu den nachfolgenden Lavaeffusionen. Gleichzeitig änderte sich auch die Zusammensetzung der Minerale in den Laven. Der Eisengehalt von Olivin und Pyroxenen verringerte sich; Plagioklase wechselten von weniger basischen zu stärker basischen Abarten. Nach Meinung des Autors sind solche Veränderungen der Minerale in den Laven das Ergebnis einer Differentiation, die auf einer temperaturabhängigen Diffusion beruht.

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Résumé Les laves du volcan Kljutchevsky qui se sont épanchées au cours de la première effusion et originant des niveaux supérieurs du volcan, sont un peu plus acides comparées aux laves des épanchements suivants. La composition des minéraux de ces laves s'est changée simultanément. L'olivine et les pyroxénes se sont changés conformément: des plus ferrugineux vers les moins ferrugineux, et les plagioclases des moins basiques vers les espèces plus basiques. Selon la supposition de l'auteur, ces changements de la composition des minéraux des laves résultent d'une différentiation qui est la conséquence de la diffusion liée au changement de la température.

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Dedicated to Professor Dr. A.Rittmann on the occasion of his 75. birthday     

岩浆补给作用对硅质火山岩浆系统演化的制约

硅质火山喷发作为大陆地壳岩浆活动的重要表现，在研究大陆地壳形成与演化、探讨岩浆过程与动力学机制等方面具有重要的价值，其通常所表现的强烈爆炸式喷发，甚至可以导致全球性的环境和气候变迁。硅质岩浆系统在开放体系中不同来源岩浆的贡献和相互作用是目前研究的热点问题。持续的岩浆补给可以延长岩浆存储的时间，促进岩浆房的对流、岩浆的分异演化以及晶体 熔体的分离和晶粥的再活化，同时也是触发火山喷发的重要机制之一。此外，岩浆补给以及硅质岩浆的晶体 熔体演化过程也是火山喷发产物多样性的原因，导致同一火山在其活动过程中喷发产物规律性的变化，如富晶体火山岩、贫晶体火山岩、火山岩成分分层、以及复活岩穹和中央侵入体等。因此，岩浆补给作用是制约硅质火山岩浆系统演化和火山岩成分多样性的重要因素，也是活动火山监测和灾害评估的重要依据。岩石学、岩石地球化学、矿物(长石、石英、石榴子石、锆石等)同位素及成分变化，以及模拟实验、地震层析成像等研究为揭示硅质岩浆系统中的岩浆补给作用和复杂岩浆过程提供了多种视角。     

Direct ascent to the surface of asthenospheric magma in a region of convex lithospheric flexure

The stress field of oceanic lithosphere controls the distribution of submarine petit-spot volcanoes. However, the eruption sites of these petit-spot volcanoes are considered to be limited to concavely flexed regions of lithosphere off the outer rise. Here, we present new data for a recently identified petit-spot lava field on a convexly flexed section of the lithosphere adjacent to the subduction zone offshore of northeast Japan in an area containing more than 80 volcanoes. This area is marked by strongly alkaline lavas that were erupted on the convexly flexed region. As for the concavely flexed region where the petit-spots previously reported, the base of the lithosphere beneath the eruption sites is under extension, whereas the upper part of the lithosphere is under compression. This change in the stress field, from the lower to upper lithosphere, causes ascending dikes to stall in the mid-lithosphere, leading to metasomatic interaction with the surrounding peridotite. The new geochemical data of rocks and xenocrysts presented in this study indicate that strongly alkaline magmas erupted on the convexly flexed region would have ascended more rapidly through the mid-depth of lithosphere because of the extensional regime of the upper lithosphere and decreasing the degree of metasomatic reaction with the surrounding mantle peridotite. The results indicate that the degree of metasomatism and the compositional variations of petit-spot magmas are controlled mainly by the stress field of the lithosphere.     

大兴安岭北部中生代火山岩特征及岩浆演化

据火山岩岩石组合、地球化学特征、喷发旋回特征及岩浆来源,将大兴安岭北部中生代火山岩划分为三个岩浆演化旋回。晚侏罗世塔木兰沟—吉祥峰旋回火山岩为碱性系列亚碱性系列,岩浆来源于上地幔并有陆壳物质的混染;早白垩世的上库力旋回火山岩为高钾钙碱性系列,岩浆来源于地壳的部分熔融;早白垩世伊列克得旋回火山岩为碱性到亚碱性过渡系列,岩浆来自于地幔并受地壳的混染。综合研究表明,大兴安岭北部中生代火山岩形成于板内环境,早白垩世火山岩可能形成于大陆裂谷环境。     

湘东北幕阜山含绿帘石花岗闪长岩岩浆的上升速率：岩相学和矿物化学证据

出露于扬子地块东南缘的幕阜山复式岩体侵位年龄约为145Ma.该复式岩体的花岗闪长岩及其暗色微粒包体都含有独特的岩浆绿帘石.这些绿帘石呈自形晶,普遍发育熔蚀结构,部分具褐帘石核.微粒包体及花岗闪长岩中绿帘石的Ps值((100Fe3+/(Fe3++Al))均集中在26～28,TiO2含量小于0.2%,为典型的岩浆成因.岩相...     

相山铀矿田火山岩浆期后成矿热液系统

文章系统论述了相山铀矿田的成矿特征,从时空尺度对成矿物质来源进行了探讨,结合成矿的构造-岩浆-地球动力学背景分析,研究了相山火山盆地成矿热液系统的形成和演化,认为相山铀矿田成矿流体系统是受区域构造环境制约、火山岩浆期后热液系统演化的客观产物。火山岩浆期后成矿热液系统在时间上延续了大约50 Ma,但在不同时间域内其活动空间有异,并由此制约着矿田内铀矿化的时空分布。文章还对矿田内深入找矿提出了建议。     

Reactions between mantle xenoliths and host magma beneath La Palma (Canary Islands): constraints on magma ascent rates and crustal reservoirs

Spinel-bearing peridotitic mantle xenoliths from the 1949 eruption on La Palma were modified mineralogically and chemically during prolonged reaction with their host magma. The magmatism that brought the peridotites to the surface caused two distinct generations of xenolith fractures: (1) Old fractures are characterized by crystalline selvages with cumulus textures towards the host magma, or by polymineralic veins. They are accompanied by 0.9–2 mm wide diffusion zones where peridotite olivine became less forsteritic through diffusive exchange with the host magma. Old fractures represent most of each xenolith's surface. (2) Young fractures show no selvages and only narrow diffusion zones of <0.02 mm width. Calculations based on a model of Fe-Mg interdiffusion give an age of 6 to 83 years and <4 days for old and young fractures, respectively. A combination of these data with fluid inclusion barometry indicates that selvages and veins formed during xenolith transport rather than representing wall-rock reactions or mantle metasomatism. The results provide ample evidence for prolonged storage of the xenoliths in the crust, constraining a multi-stage magma ascent: Years to decades prior to eruption, ascending magma ruptured peridotitic wall-rock possibly through hydraulic fracturing and stoping around magma reservoirs. Magma batches transported the peridotite xenoliths to the crust at ascent rates exceeding 0.2 ms⁻¹. The xenoliths and their host magma stagnated during at least 6 years in possibly sill-like reservoirs at 7–11 km depth. The xenoliths became deposited and subsequently embedded in a mush of settled phenocrysts, while selvages and veins crystallized until the eruption commenced. At the end of the eruption, the xenoliths were finally transported to the surface within hours to days. Decompression during the rapid ascent induced internal stresses and caused renewed fragmentation of the xenoliths, producing the young fractures. Received: 25 August 1997 / Accepted: 25 November 1997     

琼北火山活动分期与全新世岩浆演化

琼北火山活动始于始新世以来,早第三纪火山岩以夹层隐伏于不同时期的地层中。本文新提供的琼北火山岩K-AT年龄和砂岩捕虏体热释光年龄,从年代学上确定了琼北存在全新世火山喷发活动。琼北地表火山岩从早到晚分为6期：蓬莱期(中新世)、金牛岭期(上新世)、多文岭期(早更新世)、东英期(中更新世)、道堂期(晚更新世)、雷虎岭期(全新世)。雷虎岭期又分为早晚两个亚期：雷虎岭亚期和马鞍岭亚期,它们分别属于橄榄拉斑玄武岩和石英拉斑玄武岩。火山岩稀土元素、微量元素和Sr,Nd,Pb同位素地球化学特征揭示,岩浆来自亏损地幔(DMM)和富集岩石圈或亏损地幔(DMM)与俯冲洋壳两种不同的地球化学组分混合源区。橄榄拉斑玄武岩是相对原始的地幔岩浆。橄榄拉斑玄武岩岩浆经约10％橄榄石分离结晶可以形成石英拉斑玄武岩浆。岩浆上升过程中未受明显的陆壳混染。