南祁连拉脊山口增生楔的结构与组成特征

造山带内增生楔/增生杂岩结构与组成的精细研究可为古洋盆演化和古板块构造格局重建提供最直接证据。北祁连构造带发育多条增生杂岩带,记录了阿拉善和中祁连地块之间原特提斯洋的俯冲和闭合过程,然而南祁连构造带大地构造演化长期存在争议。地质填图结果表明,南祁连构造带拉脊山口地区存在一套强烈片理化的玄武岩、灰黑色和红色硅质岩、砂岩和泥岩组合,它们与一套呈现"块体裹夹于基质"结构特征的混杂岩共同构成了增生杂岩,发育双重逆冲构造、逆冲断层、无根褶皱、紧闭褶皱和透入性面理。该增生杂岩与蛇绿岩之间为断层接触,并位于断层下盘。混杂岩是由斜长花岗岩(561Ma)、斜长岩(507Ma)、辉绿岩、玄武岩、硅质岩和砂岩等外来或原地岩块与浊流成因的细碎屑岩基质共同组成;基质和砂岩块体均发育同沉积构造,呈现出滑塌堆积典型特征。空间上,拉脊山口增生杂岩与上覆蛇绿岩被断层所分割且共同仰冲于中祁连南缘青石坡组浊积岩之上,具有与东侧昂思多地区增生杂岩和蛇绿岩相似的岩石组成、构造变形和时空结构特征。它们与南侧的岛弧带共同构成了南祁连构造带寒武纪-早奥陶世沟-弧体系,指示了寒武纪-早奥陶世时期南祁连洋盆向南俯冲。     

Strength and deformation behavior of the Shimanto accretionary complex across the Nobeoka thrust

A rapid reduction in sediment porosity from 60 to 70 % at seafloor to less than 10 % at several kilometers depth can play an important role in deformation and seismicity in the shallow portion of subduction zones. We conducted deformation experiments on rocks from an ancient accretionary complex, the Shimanto Belt, across the Nobeoka Thrust to understand the deformation behaviors of rocks along plate boundary faults at seismogenic depth. Our experimental results for phyllites in the hanging wall and shale‐tuff mélanges in the footwall of the Nobeoka Thrust indicate that the Shimanto Belt rocks fail brittlely accompanied by a stress drop at effective pressures < 80 MPa, whereas they exhibit strain hardening at higher effective pressures. The transition from brittle to ductile behavior in the shale–tuff mélanges lies on the same trend in effective stress–porosity space as that for clay‐rich and tuffaceous sediments subducting into the modern Nankai subduction zone. Both the absolute yield strength and the effective pressure at the brittle–ductile transition for the phyllosilicate‐rich materials are much lower than for sandstones. These results suggest that as the clay‐rich or tuffaceous sediments subduct and their porosities are reduced, their deformation behavior gradually transitions from ductile to brittle and their yield strength increases. Our results also suggest that samples of the ancient Shimanto accretionary prism can serve as an analog for underthrust rocks at seismogenic depth in the modern Nankai Trough.     

准噶尔盆地东部石炭纪富火山岩海相油气盆地原型:一个工作假说

准噶尔盆地石炭系中发现自生自储的大型火山岩油气藏,这不仅大大拓宽了油气勘探领域,而且从含油气盆地原型恢复角度为我们提出了一个新的命题。本文对准噶尔盆地东部的石炭纪盆地进行了剖析,在井间地层对比和锆石U-Pb同位素年代学测定基础上,确定了准噶尔盆地石炭系划分方案,建立了准东地区及邻区石炭系的5条联井对比骨干地质剖面,进而把准东地区石炭系盆地的充填过程划分为两个旋回、7个阶段,其中第一旋回为早石炭世,进一步分为4个阶段,第1至第3阶段以各种火山岩发育为特征,第4阶段为火山活动的间歇期,发育了暗色泥质岩。第二旋回为晚石炭世,进一步分为3个阶段,第5和第6两个阶段以发育中基性火山岩为特征,第7阶段以沉火山凝灰岩和与泥质岩、砂岩互层发育为特征。文中归纳了准东地区石炭纪盆地及其中火山岩油气藏烃源岩和储层的发育特点,建立了其盆地原型,指出准东地区石炭系在沉积时的构造古地理以多岛洋为特征,受准噶尔洋的持续向北东方向俯冲的影响,准东地区盆地基底向南西方向倾斜,造成了沉积中心的向南西迁移。考虑到盆地位于增生型造山带内,将其原型盆地称为增生楔盆地。文中特别指出,任何构造位置上形成的盆地都有形成大油气田的潜力,能否形成大油气田的关键在于有没有优质烃源岩、优质储层和有效圈闭。准东增生楔盆地中烃源岩与火山岩储层的空间关系十分密切,二者往往形成互层状或穿插状,这一特征决定了盆地中油气产出具有近源性,而圈闭的形成则因火山岩储层的成层性差而呈形态和类型的多样性。     

Uncertainty analysis of space–time prisms based on the moment-design method

Space–time prism (STP) is an important concept for the modeling of object movements in space and time. An STP can be conceptualized as the result of the potential path of a moving object revolving around in the three-dimensional space. Though the concept has found applications in time geography, research on the analysis and propagation of uncertainty in STPs, particularly under high degree of nonlinearity, is scanty. Based on the efficiency and effectiveness of the moment-design (M-D) method, this paper proposes an approach to deal with nonlinear error propagation problems in the potential path areas (PPAs) of STPs and their intersections. Propagation of errors to the PPA and its boundary, and to the intersection of two PPAs is investigated. Performance of the proposed method is evaluated via a series of experimental studies. In comparison with the Monte Carlo method and the implicit function method, simulation results show the advantages of the M-D method in the analysis of error propagation in STPs.     

LAMOST望远镜的大气色散校正

大气折射与大气色散会影响大视场多目标光纤光谱观测的质量和效率.一个焦距为20m,焦比为F5、位于北纬40.4°的LAMOST望远镜在中天和中天前后0.75小时产生的色散值,用模拟计算得到结果,并用数值计算得到验证.对校正色散可能用的几种色散棱镜进行了计算分析比较,确定了色散棱镜的型式,并分析了色散棱镜的二级光谱以及色散棱镜在望远镜跟踪过程中的残留色散,及色散棱镜的安装误差.     

Petrogenesis of greenstones from the Mino–Tamba belt, SW Japan: Evidence for an accreted Permian oceanic plateau

Permian greenstones in the Jurassic Mino–Tamba accretionary complex, southwest Japan, are divided into three distinct series on the basis of their geological occurrence, mineralogy, and geochemistry. A low-Ti series (LTS) is associated with Lower Permian chert and limestone, and is the most voluminous of the three series. The LTS shows slightly more enriched geochemical and isotopic characteristics than MORB. A transition series (TS) is mainly associated with Lower Permian chert, and has more enriched geochemical signatures than MORB. Its isotopic characteristics are divided into enriched and depleted types. A high-Ti series (HTS) occurs as sills and hyaloclastites within Middle Permian chert and as dikes intruding the TS. Some HTS rocks have high MgO contents. The HTS is characterized by enrichment in incompatible trace elements and an isotopic composition comparable to HIMU-type basalt. The geochemistry of the voluminous LTS is similar to that of the oceanic basalt series of the Kerguelen plateau, suggesting production by partial melting of a shallow mantle plume head below thick oceanic lithosphere in Early Permian time. We infer that the TS formed simultaneously at the margins of the mantle plume head. In contrast, the HTS may have resulted from partial melting of a deep mantle plume tail in Middle Permian time. Permian greenstones in the Mino–Tamba belt may have thus formed by superplume activity in an intra-oceanic setting. Given the presence of two known contemporary continental flood basalt provinces (Siberia and Emeishan) and some accreted oceanic plateau basalts, the vast magmatism of the Mino–Tamba oceanic plateau suggests a large-scale superplume pulse in Permian time. Accretion of oceanic plateaux may have played an important role in the growth of continental margins and island arcs in Japan and elsewhere in the circum-Pacific region.     

Embayment characteristic time and biology via tidal prism model

Transport time scales are often offered by scientists, and accepted by ecologists, as qualitative indicators of the susceptibility of ecological components within an embayment. However, rigorous quantitative methods were never presented to confirm this intuition. Transport time scales in water bodies are classically based on their physical and chemical aspects rather than their ecological and biological character. The direct connection between a physical time scale and an ecological effect has to be investigated in order to quantitatively relate a transport time scale to ecology. This concept is presented here with some general guidelines and clarifying examples. To be able to relate physical time scales to biological processes, a simple tidal prism model is developed that calculates temporal changes in concentration and the related exposure. This approach provides a quick method to calculate the characteristic time for transport in a large number of embayments, which can also help in classification endeavors.     

台湾增生楔天然气水合物的地震特征

通过对南海973航次在该区域的多道地震剖面的分析,结合该区域的地质背景,认为台湾增生楔具有天然气水合物存在和分布的地球物理特征,在地震剖面上出观海底反射层(BSR)、振幅空白(BZ)、极性反转等地震识别标志。BSR所在区域位于南海向菲律宾海板块俯冲的增生楔上,南海新生代沉积不仅提供了富含有机质的丰富物源,而且类似于活动大陆边缘的构造体系又为天然气水合物的形成提供了良好的条件。     

Progressive deformation of an evaporite-bearing accretionary complex: SeaMARC I,SeaBeam and piston-core observations from the Mediterranean Ridge

The Mediterranean Ridge is an arcuate ridge of deformed sediment caught up in the convergent plate margin between the African plate and the Aegean. An intensive campaign of SeaMARC I and SeaBeam surveys followed by piston coring has been conducted along the contact between undeformed turbidites of the Sirte Abyssal Plain and folded and faulted sediments of the Mediterranean Ridge. Along the outer edge of the Ridge, surficial sediments have been deformed into sinusoidal ridges and troughs (wavelengths 0.5–2 km, amplitude 20–150 m), which we interpret as folds. In plan view, the ridge and the trough fabric parallels the NW-SE trending regional contours, suggesting that the folds formed in response to compression orthogonal to the Mediterranean Ridge. The outermost ridge is shedding a debris apron out onto the abyssal plain, implying that uplift and deformation are ongoing. We show that the geometry of the outermost folds can be produced by elastic bending of a packet of 5–10 relatively strong layers, each 10–20 m thick, interbedded between weaker layers; we equate the strong layers with gypsum beds in the Messinian upper evaporites. Folding the seafloor from a flat layer into the observed ridge and trough topography would shorten the layer by less than 2%. Two percent shortening (equals two percent thickening) is insufficient to create the observed relief of the Mediterranean Ridge even if the entire sediment column down to basement were involved; we infer that additional shortening/thickening is accommodated by thrust faulting above a decollement at the top of the Messinian salt layer. At distances > 15 km from the deformation front and more than 500 m from the abyssal plain, sharp-edged, fine-grained side-scan lineations with very little vertical relief cut across the kilometer-scale ridge and trough topography. These fine-grained lineations fall in two groups trending N/S to NNE/SSW and ~ENE. We interpret these lineaments as traces of conjugate strike-slip faults formed in the same compressional regime which formed the NW/SE trending folds. The onset of strike-slip faulting may coincide with the cessation of imbricate thrust fan development above the initial salt-controlled decollement surface. The following characteristics of the Mediterranean Ridge are attributed to the presence of evaporites in the incoming sedimentary section: (1) initial deformation by folding rather than thrust faulting; (2) narrow taper; (3) rapid rate of outward growth; (4) karstification.     

Combining 2D-basin and structural modelling to constrain heat transport along the Muroto Transect,Nankai Trough,Japan

The Nankai Trough located southeast of Shikoku Island, Japan, exhibits a zone of exceptionally high heat flow. In the central part of the Nankai Trough the fossil spreading centre of the Shikoku Basin is subducted beneath the southwest Japan arc. We have modelled the temperature and maturation history along the Muroto Transect reaching from the tip of the thrust zone out into nearly undeformed Quaternary and Tertiary sediments seawards of Nankai Trough. We used two balanced cross-sections defining the sections before and after overthrusting as input for 2D-basin modelling. We can show that rapid burial and overthrusting during the Quaternary in combination with a heat flow history following the cooling curve of a 15 Ma old oceanic plate is not sufficient to explain the measured maturity of organic material in the sediments. Several heat flow scenarios derived from theoretical concepts [Yamano, M., Kinoshita, M., Goto, S., Matsubayashi, O., 2003. Extremely high heat flow anomaly in the middle part of the Nankai Trough. Physics and Chemistry of the Earth, Parts A/B/C 28, 487–497.] and previous modelling approaches [e.g. Brown, K.M., Saffer, D.M., Bekins, B.A., 2001. Smectite diagenesis, pore water freshening, and fluid flow at the toe of the Nankai wedge. Earth and Planetary Science Letters 194, 97–109; Spinelli, G.A., Underwood, M.B., 2005. Modeling thermal history of subducting crust in Nankai Trough: constraints from in situ sediment temperature and diagenetic reaction progress. Geophysical Research Letters 32(L09301): doi:10.1029/2005GL022793; Steurer, J., Underwood, M.B., 2003. Clay mineralogy of mudstones from the Nankai Trough reference sites 1173 and 1177 and frontal accretionary prism site 1174. In: H. Mikada et al. (Eds.), pp. 1–37. Available from: <http://www-odp.tamu.edu/publications/190196SR/VOLUME/CHAPTERS/211.PDF>] were tested. The best match between observed maturity levels, temperature and heat flow measurements is reached for a heat flow history which initially assumes the cooling of a 15 Ma old oceanic lithosphere but is reheated to 170–180 mW/m² during the phase of rapid burial in the Quaternary. This can be achieved either by assuming the onset of hydrothermal circulation in the cooling crust or by reheating caused by off-axis volcanism at about 6 Ma [Yamano, M., Kinoshita, M., Goto, S., Matsubayashi, O., 2003. Extremely high heat flow anomaly in the middle part of the Nankai Trough. Physics and Chemistry of the Earth, Parts A/B/C 28, 487–497.].