Jellyfish patch formation investigated by aerial photography and drifter experiment

Jellyfish patch formation is investigated by conducting a drifter experiment combined with aerial photography of a sustained patch of the moon jellyfish in Hokezu Bay, Japan. Jellyfish patches are aggregations of individuals that are caused by a combination of swimming (active influence) and advection by currents (passive influence). The drifter experiment involved the injection of 49 drifters around a distinct surface patch of jellyfish within an area of approximately 300 m × 300 m. The drifters’ motion, caused only by the passive influence, was recorded in a series of 38 aerial photographs taken over approximately 1 h. The ambient uniform current field larger than the patch scale was estimated from the movement of the centroid position of drifters, while the distribution of horizontal divergence and relative vorticity around the patch was estimated from the time-derivative in areas of triangles formed by the drifters. The centroid positions of both drifters and patches moved stably toward the bay head at different speeds. The difference vector between the patch and drifter centroids was directed to the sun, and was opposite to the ambient current. The distributions of vorticity and divergence around patches exhibited inhomogeneity within the patch scale, and the drifters in this nonuniform current field aggregated near the convergence area within 1 h. The results suggest that horizontal patch formation is predominantly influenced by passive factors at the surface of Hokezu Bay. Furthermore, the upward swimming against downwelling may make sustained patch in surface layer.     

Timing and development of sedimentation of the Cleaverville Formation and a post‐accretion pull‐apart system in the Cleaverville area,coastal Pilbara Terrane,Pilbara, Western Australia

In the Cleaverville area of Western Australia, the Regal, Dixon Island, and Cleaverville Formations preserve a Mesoarchean lower‐greenschist‐facies volcano‐sedimentary succession in the coastal Pilbara Terrane. These formations are distributed in a rhomboidal‐shaped area and are unconformably overlain by two narrowly distributed shallow‐marine sedimentary sequences: the Sixty‐Six Hill and Forty‐Four Hill Members of the Lizard Hills Formation. The former member is preserved within the core of the Cleaverville Syncline and the latter formed along the northeast‐trending Eighty‐Seven Fault. Based on the metamorphic grade and structures, two deformation events are recognized: D₁ resulted in folding caused by a collisional event, and D₂ resulted in regional sinistral strike‐slip deformation. A previous study reported that the Cleaverville Formation was deposited at 3020 Ma, after the Prinsep Orogeny (3070–3050 Ma). Our SHRIMP U–Pb zircon ages show that: (i) graded volcaniclastic–felsic tuff within the black shale sequence below the banded iron formation in the Cleaverville Formation yields an age of (3 114 ±14) Ma; (ii) the youngest zircons in sandstones of the Sixty‐Six Hill Member, which unconformably overlies pillow basalt of the Regal Formation, yield ages of 3090–3060 Ma; and (iii) zircons in sandstones of the Forty‐Four Hill Member show two age peaks at 3270 Ma and 3020 Ma. In this way, the Cleaverville Formation was deposited at 3114–3060 Ma and was deformed at 3070–3050 Ma (D₁). Depositional age of the Cleaverville Formation is at least 40–90 Myr older than that proposed in previous studies and pre‐dates the Prinsep Orogeny (3070–3050 Ma). After 3020 Ma, D₂ resulted in the formation of a regional strike‐slip pull‐apart basin in the Cleaverville area. The lower‐greenschist‐facies volcano‐sedimentary rocks are distributed only within this basin structure. This strike‐slip deformation was synchronous with crustal‐scale sinistral shear deformation (3000–2930 Ma) in the Pilbara region.     

中国油气页岩分布与存储潜能和前景分析

基于当今化石油气能源的需求还在扩展,它的紧缺势态波及全球,而我国的确需要更多的页岩油气.为此,非常规油气能源,特别是页岩油气的勘探、开发和利用就必然地提到社会进步和经济发展的议程上,并得到世界各个国家的高度重视.因此,页岩油气现已成为我国能源界和科技界及政府部门的热门话题.在经过了一段时间的"热炒"和依据尚不充分的评估后,本文通过对中外有关资料的分析和讨论认为:1)必须在了解世界各国、特别是北美页岩油气赋存与开发的条件下,认识我国页岩的分布状态和页岩油气潜能;2)在理解其它国家页岩属性、页岩油气的前景和勘查及储存背景下,在我国较全面的进行页岩和页岩油气存储的勘探和对其进行要素匹配,并选择远景好的典型地区进行示范研究与探索;3)集理念与实践综合研究制定页岩油气在我国的发展方案和路线图.     

火山岩风化壳地层型油气藏评价预测方法研究——以新疆北部石炭系为例

针对火山岩风化壳地层型油气藏强非均质性,评价预测难度大,勘探成功率低等难题,本文采用重磁电剥层处理、沿层延拓信号增强反演方法有效顶测区域火山岩分布;建立风化淋滤剥蚀后不同岩石组合的不完整火山机构和形态识别模式,利用相干体和振幅分析等方法有效识别火山岩目标;在建立单次火山喷发岩石序列及储层分布模式基础上,开发了基于次生溶...     

凝胶堵漏技术在阳山矿区漏失地层中的应用

甘肃省文县阳山矿区地质构造复杂,地层破碎蚀变强烈,多层位漏失,钻探施工漏失现象普遍。在研究地层漏失机理的基础上试验应用了聚合物凝胶堵漏技术。ZK2232孔的现场应用表明,聚合物凝胶堵漏剂与其他惰性桥堵剂配合使用,能很好地解决钻进过程中的恶性漏失问题,堵漏效果较好。在堵漏施工中,聚合物凝胶堵漏不受漏失通道的限制,能够通过挤压变形进入裂缝和孔洞空间,最终达到封堵漏层的目的。     

庐枞火山盆地深部岩石与成矿过程

黄铁矿-硬石膏-磁铁矿矿石为典型矿石的金属矿床产于长江中下游中生代火山盆地,庐枞火山岩盆地。丰富的铁矿和黄铁矿床,主要分布在火山岩和潜火山岩里,同时也分布于盆地周边。火山岩石主要是钾玄岩-粗安岩-粗面岩组合。在深部,与它们的成分对应的岩浆岩石是碱性辉长岩-辉石二长岩-正长岩组合,如缺口辉长岩,杨山地区的辉石正长岩。火山岩和深部的辉长岩-二长岩-正长岩都经历了多次水热活动。黄铁矿-硬石膏-磁铁矿矿床主要伴随两套蚀变,即,火山岩石的大面积深色蚀变(硬石膏-辉石-长石蚀变岩)和浅色蚀变(硅化泥化)。在二长-正长岩与火山岩石的接触带,有强烈的类云英岩石(电气石-石英-云母组合)。在缺口辉长岩里,曾经发现大量磁铁矿脉(磁铁矿-方柱石-方钠石-石榴石组合)。在杨山和马口地区,正长岩里的铁矿是辉石钾长石磁铁矿组合及阳起石-磷灰石-磁铁矿组合。二长-正长岩体在盆地里广泛分布,在大范围内是几乎是层状的。调查研究表明:火山盆地底部辉长岩-二长岩-正长岩组合与铁矿有关。盆地里深部岩石和成矿作用存在有垂直分布特性。上面是喷发岩石,及潜火山岩石,下面是深部的碱性辉长岩-二长岩-正长岩杂岩体。中间有过渡带,岩墙岩席带。上面是与钾玄岩-粗安岩层和潜火山岩石里赋存的磁铁矿和黄铁矿床,下面有产于碱性辉长岩-二长岩-正长岩里也有铁矿化。蚀变岩石地质年代的初步研究发现:罗河铁矿的深部钠长石化岩石,与马口铁矿附近的正长岩石的地质年代接近(110～119Ma)。事实说明,在火山岩和潜水火山岩石里成矿作用和深部岩浆岩里成矿作用可能是同时发生的。20～435℃条件下正长岩石与水的反应动力学实验表明,在400℃左右时正长岩最容易被溶解。正长岩与水反应后,也会形成一个携带金属的流体。水岩相互作用实验提供了认识深部岩石性质的依据,有利于理解对深部的地球物理探测结果。     

Rapid Variscan exhumation and the role of magma in core complex formation: southern Brittany metamorphic belt, France

ABSTRACT The high-grade migmatitic core to the southern Brittany metamorphic belt has mineralogical and textural features that suggest high-temperature decompression. The chronology of this decompression and subsequent cooling history have been constrained with ⁴⁰Ar/³⁹ Ar ages determined for multigrain concentrates of hornblende and muscovite prepared from amphibolite and late-orogenic granite sheets within the migmatitic core, and from amphibolite of the structurally overlying unit. Three hornblende concentrates yield plateau isotope correlation ages of c. 303–298 Ma. Two muscovite concentrates record well-defined plateau ages of c. 306–305 Ma. These ages are geologically significant and date the last cooling through temperatures required for intracrystalline retention of radiogenic argon. The concordancy of the hornblende and muscovite ages suggest rapid post-metamorphic cooling. Extant geochronology and the new ⁴⁰Ar/³⁹Ar data suggest a minimum time-integrated average cooling rate between c. 725 °C and c. 125 °C of c. 14 ± 4°C Ma^-1, although below 600 °C the data permit an infinitely fast rate of cooling. Mineral assemblages and reaction textures in diatexite migmatites suggest c. 4 kbar decompression at 800–750 °C. This must have pre-dated the rapid cooling. Emplacement of two-mica granites into the metamorphic belt occurred between 345 and 300 Ma. The youngest plutons were emplaced synkinematically along shallow-dipping normal faults interpreted to be reactivated Eo-Variscan thrusts. A penetrative, west-plunging stretching lineation developed in these granites suggests that extension was orogen-parallel. Extension was probably related to regional uplift and gravitational collapse of thermally weakened crust during constrictional (escape) tectonics in this narrow part of the Variscan orogen. This followed slab breakoff during the terminal stages of convergence between Gondwana and Laurasia; detachment may have been consequent upon a change in kinematics leading to dextral displacement within the orogen. Dextral ductile strike-slip displacement was concentrated in granites emplaced synkinematically along the South Armorican Shear Zone. Rapid cooling is interpreted to have resulted from tectonic unroofing with emplacement of granite along decollement surfaces. The high-grade migmatitic core of the southern Brittany metamorphic belt represents a type of metamorphic core complex formed during orogen-parallel extensional unroofing and regional-scale ductile flow.     

Formation and evolution of elliptical galaxies and QSO activity

We present the results of a numerical code that combines multi-zone chemical evolution with 1D hydrodynamics to follow in detail the evolution and radial behaviour of gas and stars during the formation of elliptical galaxies. We use the model to explore the links between the evolution and formation of elliptical galaxies and QSO activity. The knowledge of the radial gas flows in the galaxy allows us to trace metallicity gradients, and, in particular, the formation of a high-metallicity core in ellipticals. The high-metallicity core is formed soon enough to explain the metal abundances inferred in high-redshift quasars. The star formation rate and the subsequent feedback regulate the episodes of wind, outflow and cooling flow, thus affecting the recycling of the gas and the chemical enrichment of the intergalactic medium. The evolution of the galaxy shows several stages, some of which are characterized by a complex flow pattern, with inflow in some regions and outflow in other regions. All models, however, exhibit during their late evolution a galactic wind at the outer boundary and, during their early evolution, an inflow towards the galactic nucleus. The characteristics of the inner inflow could explain the bolometric luminosity of a quasar lodged at the galactic centre as well as the evolution of the optical luminosity of quasars.     

A numerical algorithm for dissipative Keplerian particle discs

We present a numerical algorithm designed to study the evolution of a distribution of solid particles orbiting around the Sun that could be applied to similar systems in which f _c ≤ Ω/2π, where f _c is the frequency of collisions, and Ω is the orbital angular speed. A number of sample particles are used to represent the whole system. Binary collisions are treated in a novel way using a Monte Carlo method that works as follows. Orbits are locally sampled to compute the velocity dispersion. Then the velocity vectors of the sample particles are modified according to random collisions with virtual particles which have velocities taken from a normal distribution computed using the previously found local velocity dispersion. The energy and momentum taken up by the virtual particles are redistributed among the neighbours of the sample particle undergoing the collision, so that conservation laws are satisfied. Simulations using this model give an estimation of the final distribution of inclinations and the associated evolutionary time-scale.