Hydrogeochemistry and reservoir characterization of the Konya geothermal fields,Central Anatolia/Turkey

A conceptual model with water samples from ten geothermal fields (?smil, Ilg?n (Çavu?cugöl), Tuzlukçu-Ak?ehir, Seydi?ehir and Kavakköy, Hüyük, Ere?li-Akhüyük, Kad?nhan?, Cihanbeyli, Karap?nar and Bey?ehir) in the province of Konya defined the geothermal system. Carbonates, quartzite and marbles of Paleozoic metamorphics are the reservoir rocks and the heating sources are igneous rock intrusions and geothermal gradient. The variable thermal water (CaMgHCO₃, CaSO₄, NaSO₄, CaHCO₃, CaNaHCO₃, NaCl and CaNaClHCO₃) had EC and temperature between 177.8 and 56,100 μS/cm and between 18.3 and 44 °C, respectively. Ca²⁺ in geothermal fluids are associated with marble and carbonate rocks and the high chloride shows direct connection with deep geothermal system, and prolonged contact with evaporite rocks. Sulphate originates from dissolution of and oxidation of sulphate and sulphur-bearing minerals. The high As, B, F and Mn concentration in some thermal water samples were determined as 85 μg/l, 148.56 mg/l, 3.01 mg/l and 208.13 mg/l, respectively. Reservoir temperatures computed by Na/K geothermometers were between 85.37–158.89 °C for Ak?ehir thermal waters and 58.78–90.45 °C for Ere?li thermal waters. The maximum reservoir temperature of other geothermal waters was 75 °C by the silica geothermometers.     

新城金矿稳定同位素地球化学特征及成矿物质的来源

新城金矿是胶东金矿集区招远—莱州成矿带的一个"焦家式"蚀变型金矿床。本文主要通过C、H、O、S、Pb同位素研究,对新城金矿成矿流体、物质来源和成矿作用进行探讨和研究。新城金矿矿石中δD值范围为-116‰~-91‰,δ18O水值范围为3.8‰~7.2‰,表明成矿流体早期来源于岩浆水,成矿晚期混入大气降水。矿石硫化物、郭家岭花岗闪长岩、玲珑花岗岩和胶东群δ34S平均值分为7.9‰、6.5‰、8.5‰和6.2‰,认为矿石硫具有对矿区地层及岩浆岩硫的继承性。硫化物矿石206Pb/204Pb=17.115~17.414,207Pb/204Pb=15.460~15.577,208Pb/204Pb=37.912~38.196,显示铅具有壳幔混合来源的特征。碳、氢、氧、硫、铅同位素反映新城金矿成矿物质和流体主要来源于深部岩浆。     

金属矿床的成矿流体成分和流体包裹体

自然界中的成矿流体按其主要成分,可分为:(1)岩浆,即形成岩浆矿床的岩浆;(2)以H2O为主的流体(含Na Cl);(3)以CO2为主的流体。地壳中的流体类型很多,只有含一定金属元素含量的,并且达到一定浓度时才称为金属矿床的成矿流体。基于对矿床中流体包裹体和天然成矿流体中金属种类和含量的测定,这些金属矿床的成矿流体按金属元素含量可以分为五组,成矿流体可以来自岩浆、岩浆热液、大气降水、盆地卤水和变质流体等地质环境。     

联合剖面法在地下热水勘探中的应用

联合剖面法是勘查地下热水中一种比较简便的方法,近年来得到了广泛应用。应用此法并结合区域地质和构造特征,了解地热田地质结构、热储、盖层、热储类型等。根据联合剖面装置获得的低阻正交点,推断出断裂构造的位置,为确定井位及温泉开发利用提供重要依据。     

地质流体对砂岩储层黏土矿物的影响——以渤海海域古近系为例

根据偏光显微镜、扫描电镜和X-衍射等分析手段获取的数据和资料,分析对比了早期沉积水介质、幔源CO2流体、大气水、超压流体和充注烃类等对储层黏土矿物的控制作用。研究表明,早期沉积水介质是储层黏土矿物的决定性因素,微咸水-半咸水湖盆储层黏土矿物以伊利石为主,淡水湖盆储层黏土矿物以高岭石为主;幔源CO2流体侵位后带来明显的储层改造和热波动效应,储层中I/S中S%含量低于同深度泥岩,储层中高岭石含量明显偏高。欠压实超压储层中黏土演化明显滞后,表现在I/S中S%含量低于同深度泥岩和常压储层。油气层高岭石含量往往远高于相近深度的水层,可能与充注烃类携带的有机酸的溶蚀作用有关,另外,烃类充注后形成的惰性成岩环境也有利于高岭石的保存,高岭石的高含量带常与油层及高渗层相对应;受大气水淋滤的储层,以长石大量溶蚀,富含高岭石为特征,储层孔隙度一般较高。     

CSAMT在碎屑岩地区地热勘查中的应用

碎屑岩因质软,导水、储水条件不良,通常作为地热有利保温盖层,而碎屑岩电阻率普遍低,厚度大的情况下形成低阻屏蔽层,勘探下伏有利储层难度极大,寻找碎屑岩中构造裂隙水是最佳的选择。但碎屑岩中的储水构造与围岩电阻率差异小,构造迹象微弱,因此在碎屑岩地区找地热技术含量较高。茅山镇位于句容盆地东缘茅山西侧,沉积了厚度超过1800m的白垩系碎屑岩,水文地质条件较差,本文应用CSAMT大范围普查、小范围精细查证布置方式,采用磁场插值校正的技术手段、收发距选取优先保证信噪比的思路,控制白垩系碎屑岩中储水断裂构造,克服低阻的碎屑岩地区构造异常微弱的难点。钻探验证结果表明,CSAMT可以经济有效地应用于碎屑岩地区地热勘查。     

江西大湖塘超大型钨矿初始岩浆流体出溶——来自似伟晶岩壳的记录

江西大湖塘地区是江南造山带中段九岭矿集区内近年查明的世界级超大型钨矿产地,白钨矿体主要呈细脉浸染状缓倾于中粗粒黑云母花岗闪长岩中。位于区内一矿带的成矿母岩顶部发育完好的似伟晶岩壳,壳层的组构特征明显,由母岩向含矿围岩,依次为似斑状黑云母花岗岩→长英质细晶岩→石英长石似伟晶岩→长石石英似伟晶岩→含白钨矿黑云母花岗闪长岩。壳内石英的阴极发光岩相学研究显示,石英巨晶、斑晶、基质和石英脉大多经历了早阶段主晶石英,中阶段扩散交代石英和晚阶段渗滤充填石英3个生长阶段。微量元素研究表明,早阶段石英的生长是一个流体加速沉淀的过程,中阶段和晚阶段流体对主晶石英均有叠加改造,其微量元素呈降低趋势。各类石英均表现为富碱金属元素、中高温（≥483℃）、低Li/Al（0.01~0.50,大多小于0.24）的地球化学特征,反映了成矿流体为岩浆水来源,石英的生长具有岩浆—热液过渡性质。综合研究表明,大湖塘一矿带似伟晶岩壳是初始含矿岩浆流体出溶的产物,其形成过程中动态的物理化学条件促进了成矿元素W由母岩向围岩搬运富集。     

鲁北临盘地热资源特征及开发利用

鲁北临盘地热资源丰富 ,热储层为新近纪黄骅群馆陶组 ,热储盖层为新近纪黄骅群明化镇组和第四纪平原组 ,热源主要来自地壳深部正常热流传导。目前已钻凿 2口地热井 ,开发利用效益显著。地热开发要避开油气层 ,石油开发要防止污染地热储水层。     

Stable isotopic signatures of superposed fluid events in granulite facies marbles of the Rauer Group, East Antarctica

The role of volatiles in the stabilization of the lower (granulite facies) crust is contentious. Opposing models invoke infiltration of CO₂-rich fluids or generally vapour-absent conditions during granulite facies metamorphism. Stable isotope and petrological studies of granulite facies metacarbonates can provide constraints on these models. In this study data are presented from metre-scale forsteritic marble boudins within Archaean intermediate to felsic orthogneisses from the Rauer Group, East Antarctica. Forsteritic marble layers and associated calcsilicates preserve a range of ¹³C- and ¹⁸O-depleted calcite isotope values (δ¹³C= -9.9 to -3.0% PDB, δ¹⁸O = 4.0 to 12.1% SMOW). A coupled trend of ¹³C and ¹⁸O depletion (～2%, ～5%, respectively) from core to rim across one marble layer is inconsistent with pervasive CO₂ infiltration during granulite facies metamorphism, but does indicate localized fluid-rock interaction. At another locality, more pervasive fluid infiltration has resulted in calcite having uniformly low, carbonatite-like δ¹⁸O and δ¹³C values. A favoured mechanism for the low δ¹⁸O and δ¹³C values of the marbles is infiltration by fluids that were derived from, or equilibrated with, a magmatic source. It is likely that this fluid-rock interaction occurred prior to high-grade metamorphism; other fluid-rock histories are not, however, ruled out by the available data. Coupled trends of ¹³C and ¹⁸O depletion are modified to even lower values by the superposed development of small-scale metasomatic reaction zones between marbles and internally folded mafic (?) interlayers. The timing of development of these layers is uncertain, but may be related to Archaean high-temperature (>1000d?C) granulite facies metamorphism.     

Full Causal Bulk Viscous LRS Bianchi I With Time Varying Constants

In this paper we study the evolution of a LRS Bianchi I Universe, filled with a bulk viscous cosmological fluid in the presence of time varying constants “but” taking into account the effects of a c-variable into the curvature tensor. We find that the only physical models are those which “constants” G and c are growing functions on time t, while the cosmological constant Λ is a negative decreasing function. In such solutions the energy density obeys the ultrastiff matter equation of state i.e. ω = 1.