青海省宗马海湖地区始新—中新统干柴沟组沉积相探析

宗马海湖地区位于柴达木盆地的北缘,有着良好的油气、钾盐勘探前景。该文在分析柴达木盆地北缘宗马海湖地区区域地质背景的基础上,对始新-中新统干柴沟组的岩石学特征、地层特征、沉积构造特征及沉积相等进行了较为深入的研究。干柴沟组沉积相以滨湖亚相、浅湖亚相及扇三角洲相为主,滨-浅亚湖沉积发育最为广泛。扇三角洲相具牵引流、重力流沉积特征,中、粗粒碎屑岩为主;滨湖亚相具较高流态的水动力条件,以砂和粉砂为主,砂泥间互层频繁;浅湖亚相以泥质沉积为主,显示低能的浅水静态沉积作用。文中总结了研究区干柴沟组沉积期沉积相演化特征,建立了干柴沟沉积相平面展布图;干柴沟组沉积相的形成与季节性变化息息相关,湖水上涨、后退导致北部山区扇三角洲较发育,而南部区域始终位于滨、浅湖环境中。     

山东临清地热田地热地质特征

山东省临清地热田主体位于冠县凹陷内,面积约1550km2。地热类型属层状孔隙型,热源是地球内部的传导热,盖层是第四系和新近纪明化镇组。可被利用的热储层有4个,最有开发利用价值的是馆陶组下段热储,该热储层顶板埋深约1100m,底板埋深约1700m,热储层厚度530~580m,含水层累积厚度158~175m,单井涌水量1500~2000m3/d,出口水温62~67℃,矿化度5000mg/L左右,具腐蚀性,结垢性弱,具较好的开发利用价值。经计算馆陶组热储层单井1a的可采量为5.431×105m3,100a可采量所释放的总热量为1.156×1013kJ,合理井距为1500m。     

重庆温泉研究进展

文章通过综述当前重庆温泉研究的相关文献,总结了前人在重庆温泉形成的地质背景、分布状况、类型、水化学特征及形成机制等方面的研究现状,并分析了重庆温泉研究和开发利用中存在的问题。重庆温泉中人工揭露较自然出露多,温度以中低温为主,泉口流量集中于10~50 L/s,色度、浊度小,水化学类型受围岩性质影响,以SO4-Ca型为主。其形成过程为:大气降水在大巴山脉及川东褶皱带背斜顶端碳酸盐岩出露区域渗入地下深部,被地温加热后沿褶皱带背斜轴部向南移动,在河谷深切处或断裂构造处出露形成温泉。重庆温泉的开发利用存在环境污染、资源利用不合理、开发不力等问题,认为应当加强温泉形成机理、温泉资源评价与保护、温泉水系统数值模拟、温泉废水处理等方面的研究,以确保温泉水资源的可持续利用。      

浅析贵州册亨县百地金矿构造特征及形成机制

从矿区（床）级别的构造尺度入手,通过总结分析,认为矿区由一个小型帚状构造及一个小型反S型构造组成,并对其形成机制进行了浅析。     

周老镇钻孔砾石层重矿物特征及地质意义

利用江汉平原周老镇钻孔的岩心样品,分析研究了钻孔岩心沉积物10层砾石层中填充物的重矿物组分及分布特征。结果显示周老镇钻孔10个砾石层自下而上可以分为3个矿物段。对比3个阶段稳定重矿物、非稳定重矿物的变化特征:阶段Ⅰ、阶段Ⅱ,沉积物主要以近源物质为主,含有少量的远源物质;而阶段Ⅲ,沉积物主要以远源物质为主,含有少量的近源物质。结合周老镇钻孔岩性及钻孔砾石含量和江汉平原第四系岩相剖面特征,判断在阶段Ⅲ,深度112.30～109.05m(1.17～1.12MaB.P.)处,钻孔沉积环境发生了重大改变,江汉平原水系发生重要调整,长江三峡贯通形成。     

长岭凹陷潜在地热初步探讨

根据长岭凹陷石油井地温测量和物探资料,从地热形成的4要素——储、盖、通、源以及地热具备的地质特征入手,分析了长岭凹陷潜在着地热资源。目前长岭盆地基本具备了储和盖,需要进一步寻找的是通和源。     

Relative velocities among accreting planetesimals in binary systems: The circumprimary case

We investigate classical planetesimal accretion in a binary star system of separation ab?50 AU by numerical simulations, with particular focus on the region at a distance of 1 AU from the primary. The planetesimals orbit the primary, are perturbed by the companion and are in addition subjected to a gas drag force. We concentrate on the problem of relative velocities Δv among planetesimals of different sizes. For various stellar mass ratios and binary orbital parameters we determine regions where Δv exceed planetesimal escape velocities vesc (thus preventing runaway accretion) or even the threshold velocity vero for which erosion dominates accretion. Gaseous friction has two crucial effects on the velocity distribution: it damps secular perturbations by forcing periastron alignment of orbits, but at the same time the size-dependence of this orbital alignment induces a significant Δv increase between bodies of different sizes. This differential phasing effect proves very efficient and almost always increases Δv to values preventing runaway accretion, except in a narrow eb?0 domain. The erosion threshold Δv>vero is reached in a wide (ab,eb) space for small <10-km planetesimals, but in a much more limited region for bigger ?50-km objects. In the intermediate vesc<Δv<vero domain, a possible growth mode would be the type II runaway growth identified by Kortenkamp et al. [Kortenkamp, S., Wetherill, G., Inaba, S., 2001. Science 293, 1127-1129].     

Fluid dynamics of local martian magma oceans

The evolution of a melt region produced by a large impact during Mars formation is addressed. While some impact induced melt is redistributed during crater excavation, sufficiently large impacts (much larger than basin forming impacts) generate an intact melt region which is retained beneath the excavation zone, i.e., a local magma ocean. Local magma ocean evolution depends on the effective rheology controlling large scale deformation of the solid part of the planet, mechanism of crystallization, and melt region size. Within the uncertainties of various parameters, two scenarios are possible. For sufficiently weak rheology or large melt region size, evolution is characterized by rapid extrusion and formation of a global magma ocean. For sufficiently strong rheology or small melt region size, in situ crystallization to a partially molten solid state occurs prior to isostatic adjustment. Subsequent to in situ crystallization, local magma ocean evolution depends on melt region size and efficiency of lateral redistribution compared to bulk conductive cooling. For large melt regions, lateral spreading occurs via plastic deformation and results in an asymmetric, global, partial melt layer. For small melt region size, viscous spreading viscous can result in bulk cooling below the solidus prior to formation of a global layer. A hypothesis for the origin of the hemispherical crustal dichotomy and Tharsis rise is suggested. The dichotomy is associated with a global partial melt layer produced by evolution of a large, local magma ocean. After dichotomy formation, evolution of a second, smaller, local magma ocean is related to Tharsis development.     

Anisotropy and rotation in homeoidally striated Jacobi ellipsoids

In this paper a unified theory of systematically rotating and peculiar motions is developed for homeoidally striated Jacobi ellipsoids, where both real and imaginary rotations are considered. The effect of positive or negative residual motion excess along the equatorial plane is considered to be equivalent either to an additional real or an imaginary rotation, respectively. The principle results consist of (i) the discovery that homeoidally striated Jacobi ellipsoids always admit an adjoint configuration i.e. a classical Jacobi ellipsoid of equal mass and axes; (ii) the establishment of further constraints on the amount of residual velocity anisotropy along the principal axes for triaxial configurations; (iii) the finding that bifurcation points from axisymmetric to triaxial configurations occur as in classical Jacobi ellipsoids, contrary to earlier findings. An interpretation of recent results from numerical simulations on stability is provided in the light of the model. (© 2006 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)