勃利盆地中生界地质特征与油气资源量计算

黑龙江省东部勃利盆地在早白垩世为陆缘断陷盆地。经晚白垩世和新近纪的构造反转改造后，呈改造残留型含油气、含煤盆地。该盆地在下白垩统发育有厚度较大的暗色泥岩和多套煤系地层。盆地内源岩有机质以生气为主，煤系地层为重要的气态烃的来源。在研究了勃利盆地中生界地质特征的基础上，运用蒙特卡罗法初步估算了盆地内的油气资源量，得出盆地油气资源量的概率分布函数图，取得不同概率下的油气资源量值。盆地的中部断陷为有利含油气区。研究结果为进一步在松辽盆地外围寻找油气资源提供了参考依据。     

红透山矿床变质岩系褶皱构造特征浅析

红透山式铜-锌矿床形成于太古代克拉通裂谷槽盆中海底火山喷发-沉积环境。因此，矿床的空间展布严格受特定的含矿岩系所控制。槽盆构造中的岩层褶皱构造最发育，矿床赋存在具多期褶皱构造叠加的大型同倾向形褶皱内，褶皱的层间虚脱是控矿有利构造空间，可以借此预测矿体侧伏方向及赋存部位。     

濮阳市地热资源特征

本文根据钻探资料和近年的勘查研究成果,结合部分已开发利用地热资源情况,对濮阳市地热资源的分布特征、赋存规律和地热田的结构进行了初步分析。指出濮阳市地热资源的分布在平面上可分为3个区,即西区、中区和东区。西区平均地温梯度为3 5℃/100m,地下热水主要储存于奥陶系马家沟组灰岩溶洞溶隙中,温度>60℃,而30～60℃的温水和温热水储存于上第三系明化镇组砂岩裂隙孔隙之中,埋深300～1080m;中区和东区的地热资源主要储存于上第三系馆陶组和明化镇组砂岩裂隙孔隙之中,中区平均地温梯度为3 2℃/100m,东区平均地温梯度为2 8℃/100m,地下热水埋藏深度在中区和东区依次加深。文中还对濮阳市地热田的储、盖、通、源等主要条件及其形成特征进行了论述。     

A Sequence of Pan-African and Hercynian Events Recorded in Zircons from an Orthogneiss from the Hercynian Belt of Western Central Iberia--an Ion Microprobe U-Pb Study

Sensitive high-resolution ion microprobe U–Pb dating showsthat a biotite orthogneiss from the Hercynian belt of westerncentral Iberia contains 1000–300 Ma zircon. Older, 1000–570Ma ages within this range represent inherited, detrital materialamong which four age components may be recognized:     

Transformation of garnet epidote amphibolite to eclogite, western Dabie Mountains, China

Omphacite and garnet coronas around amphibole occur in amphibolites in the Hong'an area, western Dabie Mountains, China. These amphibolites consist of an epidote–amphibolite facies assemblage of amphibole, garnet, albite, clinozoisite, paragonite, ilmenite and quartz, which is incompletely overprinted by an eclogite facies assemblage of garnet, omphacite and rutile. Coronas around amphibole can be divided into three types: an omphacite corona; a garnet–omphacite–rutile corona; and, a garnet–omphacite corona with less rutile. Chemographic analysis for local reaction domains in combination with petrographical observations show that reactions Amp + Ab + Pg = Omp +Czo + Qtz + H₂O, and Amp + Ab = Omp ± Czo + Qtz + H₂O may lead to the development of omphacite coronas. The garnet–omphacite–rutile corona was formed from the reaction Amp + Ab + Czo + Ilm ± Qtz = Omp + Grt + Rt + H₂O. In garnet–omphacite coronas, the garnet corona grew during an early stage of epidote amphibolite facies metamorphism, whereas omphacite probably formed by the reactions forming the omphacite corona during the eclogite facies stage. It is estimated that these reactions occurred at 0.8–1.4 GPa and 480–610 °C using the garnet–clinopyroxene thermometer and omphacite barometer in the presence of albite.     

Grain coarsening in contact metamorphic carbonates: effects of second-phase particles, fluid flow and thermal perturbations

Under contact metamorphic conditions, carbonate rocks in the direct vicinity of the Adamello pluton reflect a temperature‐induced grain coarsening. Despite this large‐scale trend, a considerable grain size scatter occurs on the outcrop‐scale indicating local influence of second‐order effects such as thermal perturbations, fluid flow and second‐phase particles. Second‐phase particles, whose sizes range from nano‐ to the micron‐scale, induce the most pronounced data scatter resulting in grain sizes too small by up to a factor of 10, compared with theoretical grain growth in a pure system. Such values are restricted to relatively impure samples consisting of up to 10 vol.% micron‐scale second‐phase particles, or to samples containing a large number of nano‐scale particles. The obtained data set suggests that the second phases induce a temperature‐controlled reduction on calcite grain growth. The mean calcite grain size can therefore be expressed in the form D = C₂ e^Q*/RT(d_p/f_p)^m*, where C₂ is a constant, Q* is an activation energy, T the temperature and m* the exponent of the ratio d_p/f_p, i.e. of the average size of the second phases divided by their volume fraction. However, more data are needed to obtain reliable values for C₂ and Q*. Besides variations in the average grain size, the presence of second‐phase particles generates crystal size distribution (CSD) shapes characterized by lognormal distributions, which differ from the Gaussian‐type distributions of the pure samples. In contrast, fluid‐enhanced grain growth does not change the shape of the CSDs, but due to enhanced transport properties, the average grain sizes increase by a factor of 2 and the variance of the distribution increases. Stable δ¹⁸O and δ¹³C isotope ratios in fluid‐affected zones only deviate slightly from the host rock values, suggesting low fluid/rock ratios. Grain growth modelling indicates that the fluid‐induced grain size variations can develop within several ka. As inferred from a combination of thermal and grain growth modelling, dykes with widths of up to 1 m have only a restricted influence on grain size deviations smaller than a factor of 1.1. To summarize, considerable grain size variations of up to one order of magnitude can locally result from second‐order effects. Such effects require special attention when comparing experimentally derived grain growth kinetics with field studies.     

开封大雾气候特征及预报

利用1961～2000年气象资料，分析了开封市大雾天气分布规律、天气特征，并总结出大雾产生的几种天气形势，找出预报指标。     

昆仑Ms 8.1地震前青藏块体北、东缘水平运动变形的关联特征

青藏块体东北缘和川滇GPS监测区1991(1993)、1999和2001年高精度GPS观测资料揭示：2001年11月14日昆仑Ms8．1地震前，青藏块体北、东缘构造区域水平运动变形场动态演变具有一定的关联性特征。即：在继承性运动总体背景下，临近大震发生时两区域运动强度同步减弱且变形状态发生变化。结合地质构造分析研究认为，昆仑Ms8．1地震前，青藏块体边界运动变形的关联性变化与大震孕育后期大范围应力应变快速积累所形成的扰动应力场有关；随着块体内部大震的发生、应变能的大量释放和构造应力场的调整，可能会促使块体边界地带具有较高应变积累的相关构造部位(尤其是未被历史强震破裂贯通的地带)的应力应变的进一步积累或破裂释放。     

鲁东南岚山头超高压变质岩流体包裹体特征与板片折返史

鲁东南岚山头含柯石英榴辉岩主要产于花岗质片麻岩内,是苏鲁超高压变质带主要榴辉岩体密集分布区之一。流体包裹体研究表明,榴辉岩矿物及细脉石英中捕获有四种类型包裹体:在超高压-高压榴辉岩相条件下捕获的 N_2±CO_2包裹体;在高压榴辉宕重结晶阶段被捕获的 CO_2-H_2O 包裹体和含子矿物高盐度 H_2O 溶液包裹体:在超高压岩石折返过程中的最晚(角闪岩相退变质甚至更晚)阶段捕获的低盐度 H_2O 溶液包裹体。利用榴辉岩矿物及脉体石英中捕获的流体包裹体相互期次关系,可以对本区超高压变质作用板片折返过程中的流体演化史进行重建。     

中国中西部前陆盆地的地质特征及油气聚集

中国中西部前陆盆地具有十分丰富的油气资源,近年来油气勘探也取得了很大的成果,但总体上来说其地质情况复杂、研究程度较低。世界上典型的前陆盆地一般位于造山带和稳定的克拉通之间的狭长槽地,而在中国中西部则主要为与古特提斯造山带在新特提斯阶段再活动有关的陆内会聚形成的“再生”前陆盆地,因此与世界典型前陆盆地相比中国中西部前陆盆地具有一定的“特殊性”。根据两期前陆的叠合程度差异造成的盆地几何形态、挠曲沉降、地层层序、沉积充填、构造变形特征的特点,将中国中西部前陆盆地归纳为改造型、新生型、叠加型和早衰型四种组合类型的前陆盆地。中西部不同组合类型前陆盆地具有不同的结构特征,决定了不同组合类型前陆盆地成藏特征和油气勘探潜力上的差异。