全安盆地水文地质特征及热水成因分析

在简要分析全安盆地水文地质特征、地下水赋存条件及划分地下水类型基础上,对盆地西部周地—暖水塘地区地下热水形成原因、赋存环境进行研究,认为多期次构造运动形成的断裂、裂隙沟通深部地下热水是盆地热水来源的主要原因;采取地下热水样品并开展氢氧稳定同位素、逸出气体、水化学成份测试,认为地下热水由大气降水补给,长期水动态观测结果也显示大气降水与地下热水关系较密切。     

贵州省瓮福磷矿沉积环境及矿床成因探讨

瓮福磷矿沉积的有利场所是潮下海湾浅滩环境,而不是潮坪。海湾的大小又控制着矿床的规模,海滩能量的差异影响着磷矿石的不同结构成因类型。矿石的结构,从凝胶―细砂屑与砂屑颗粒由细变粗;岩石的颜色由灰褐、黑色(多陆屑、富有机炭及黄铁矿)变为浅灰、灰白色;矿层中P2O5含量随之渐增,而且CaO含量变化与P2O5含量变化同步,说明水动力条件由弱渐强,反映了沉积环境由潮汐作用为主的海湾环境。为此,陡山沱组以浅水碳酸盐优势岩相的地层条件是成磷的前提;温暖、干燥的古气候提供了有利于磷质的析出及沉积;适宜的海滩古地理环境提供了最佳的成矿场所;"黔中隆起"的古构造条件是磷矿的分布及富矿形成的最主要的控制因素。     

大兴安岭北段塔源二支线铅锌铜矿区岩浆岩岩石成因及其地质意义

塔源二支线铅锌铜矿床地处额尔古纳地块东南缘,位于得尔布干成矿带东段.为确定塔源二支线铅锌铜矿区岩浆岩的岩石成因及其地质意义,对矿区岩浆岩开展了岩石学、地球化学以及同位素年代学研究.笔者在矿区识别出两期岩浆作用,早期发生于(296.1±2.3)Ma(早二叠世),侵入体为二长闪长岩;晚期发生在(136.5±2.1)Ma(早...     

On the hydraulic intake shape factor for a circular opening located at an impervious boundary: Influence of inclined stratification

In this paper, we develop an exact closed form solution for a circular entry point located at the interface between an impermeable material and a stratified porous medium, where the principal plane of hydraulic isotropy is inclined to the interface. Copyright © 2010 John Wiley & Sons, Ltd.     

Hubble Space Telescope imaging of the progenitor sites of six nearby core-collapse supernovae

The search for the progenitors of six core-collapse supernovae (CCSNe) in archival Hubble Space Telescope ( HST ) WFPC2 pre-explosion imaging is presented. These SNe are 1999an, 1999br, 1999ev, 2000ds, 2000ew and 2001B. Post-explosion imaging of the SNe, with the HST ACS/WFC, has been utilized with the technique of differential astrometry to identify the progenitor locations on the pre-explosion imaging. SNe 1999br, 1999ev, 2000ew and 2001B are recovered in late-time imaging, and estimates of the progenitor locations on the pre-explosion imaging, with subpixel accuracy, have been made. Only the progenitor of the Type II-P SN 1999ev has been recovered, on pre-explosion F555W imaging, at a 4.8σ significance level. Assuming a red supergiant progenitor, the pre-explosion observation is consistent with   M _ZAMS= 15–18 M_⊙  . The progenitors of the other five SNe were below the 3σ detection threshold of the pre-explosion observations. The detection thresholds were translated to mass limits for the progenitors by comparison with stellar evolution models. Pre-explosion observations of the peculiarly faint SN 1999br limit the mass of a red supergiant progenitor to   M _ZAMS < 12 M_⊙  . Analysis has been extended, from previous studies, to include possible detections of high- T _eff, high-mass stars by conducting synthetic photometry of model Wolf–Rayet star spectra. The mass limits for the Type II-P SNe 1999an and 1999br are consistent with previously determined mass limits for this type of SN. The detection limits for the progenitors of the Type Ibc SNe (2000ds, 2000ew and 2001B) do not permit differentiation between high-mass Wolf–Rayet progenitors or low-mass progenitors in binaries.     

Influence of underground space development mode on the groundwater flow field in Xiong’an new area

The degree and scale of underground space development are growing with the continuous advancement of urbanization in China. The lack of research on the change of the groundwater flow field before and after the development of underground space has led to various problems in the process of underground space development and operation. This paper took the key development zone of the Xiong’an New Area as the study area, and used the Groundwater modeling system software (GMS) to analyse the influence on the groundwater flow field under the point, line, and surface development modes. The main results showed that the underground space development would lead to the expansion and deepening of the cone of depression in the aquifer. The groundwater level on the upstream face of the underground structure would rise, while the water level on the downstream face would drop. The “line” concurrent development has the least impact on the groundwater flow field, and the maximum rise of water level on the upstream side of the underground structure is expected to be approximately 3.05 m. The “surface” development has the greatest impact on the groundwater flow field, and the maximum rise of water level is expected to be 7.17 m.     

鄂尔多斯盆地延长探区低渗致密油气成藏理论进展及勘探实践

延长石油集团在鄂尔多斯盆地大力推动石油、天然气、页岩气勘探开发理论研究和技术攻关,多类型资源协同发展,取得显著效果。在石油勘探方面,提出延长组特低渗石油“交替式”成藏理论认识,建立盆地中生界多期差异性成藏新模式,近10年特低渗石油年均探明地质储量超1×10⁸ t。建立细粒沉积风暴、地震等控砂理论,以及甜点预测方法,致密油累计探明地质储量2.1×10⁸ t。针对致密气田砂体成因机理不明、天然气运聚成藏规律不清等主要难题,揭示了“浅水环境岸线频繁迁移控砂”机制,建立了致密砂岩气优质储层成储模式,明确纯石英砂岩和富石英低塑性颗粒岩屑砂岩是致密气分布的“甜点”,形成了基于多要素、全过程天然气运聚模拟的目标优选技术。经勘探实践,发现了延安气田,累计探明天然气地质储量7 635×10⁸ m³。页岩气方面,提出陆相页岩气“三元”成藏富集地质理论的创新认识,认为湖相优质页岩是陆相页岩气富集高产的物质基础,多类型、跨尺度的复杂孔隙网络决定页岩气赋存条件,厚层页岩自封闭能力及高压是保存的关键,实现陆相页岩气产量突破。未...     

大兴安岭地区古生代构造格架重建:来自俯冲增生杂岩研究进展

大兴安岭地区古生代处于古亚洲洋闭合阶段,其间发育众多的弧盆系和蛇绿岩带,笔者等在大兴安岭地区1: 1 000 000地质编图和野外地质调研基础上,应用“洋板块地质”学术思想在大兴安岭地区元古宙、古生代地质体中划分出一系列“俯冲增生杂岩”、地块基底残块、岛弧、弧前盆地、弧后盆地等构造单元,结合陆(地)块和岩浆弧、弧前盆地、弧后盆地和“俯冲增生杂岩”的时空展布,划分出9条俯冲增生杂岩带,其中新识别出3条俯冲增生杂岩带。俯冲增生杂岩带主要分布于兴蒙造山带内部各地块之间和地块与大型岛弧带之间,相当于地块间及地块与岛弧带间的缝合带。依据俯冲增生杂岩带两侧对应的陆(地)块、岛弧带等构造级别,归并出5条结合带。俯冲增生杂岩带的展布方向以北东向为主,时代自北向南依次变新,从早奥陶世演化到中—晚二叠世,暗示古亚洲洋洋盆向大兴安岭地区陆(地)块俯冲作用最早发生在北部额尔古纳一带,逐渐向南后撤,不断形成新的洋壳和产生俯冲增生作用,相应的活动陆缘从北部额尔古纳地块向南逐渐增生,配套弧盆系时代也逐渐向南变新。早—中三叠世至西拉木伦一带发生陆-陆拼贴,完成华北板块与西伯利亚板块的对接。通过对大兴安岭地区古生代“俯冲增生杂岩”的研究,重建了大兴安岭地区古生代构造格架,提高了古亚洲洋东段洋-陆转换的研究程度。     

大兴安岭中生代火山岩地层时空分布与蒙古—鄂霍茨克洋、古太平洋板块俯冲作用响应

为了提高大兴安岭中生代火山岩地层的区域可对比性、深入研究大兴安岭中生代火山岩与古太平洋和蒙古—鄂霍茨克洋的构造关系,本文在大兴安岭地区1: 1 000 000地质图编图的基础上,依据岩石组合、古生物、接触关系、区域对比以及最新的年代学(锆石U-Pb、⁴⁰Ar/³⁹Ar测年)资料,对大兴安岭中生代火山岩地层重新进行了厘定。进一步界定了塔木兰沟组(172~161 Ma)、满克头鄂博组(162~148 Ma)、玛尼吐组(158~145 Ma)、白音高老组(145~129 Ma)、梅勒图组(143~128 Ma)、龙江组(128~120 Ma)、光华组(128~118 Ma)、甘河组(120~113 Ma)和孤山镇组(118~110 Ma)的形成时代。结合古太平洋、蒙古—鄂霍茨克洋板块对东亚大陆边缘的俯冲作用,解析了中生代火山岩形成的构造背景,认为中—晚侏罗世NE向展布的火山岩主要形成于蒙古—鄂霍茨克洋板块向南东俯冲的伸展背景,早白垩世NNE向展布的火山岩主要形成于伊泽奈岐板块向东亚大陆俯冲的伸展背景。晚侏罗世与早白垩世火山岩地层之间发育的开库康组、木瑞组等类磨拉石建造,是两个构造体系转换阶段的主要沉积记录。     

雄安新区D01井岩溶热储下伏太古界中热流测定研究

【研究目的】目前雄安新区范围内的热流数据多测自于新近系沉积盖层及白云岩地层,对岩溶热储下伏太古界的热流测定研究还鲜见报道,主要受限于以往的地热勘查开发层位主要在1800m以浅的蓟县系岩溶热储,揭露岩溶热储下伏太古界的钻孔稀少。2018年以来,在雄安新区牛驼镇地热田实施了D01深部地热参数井,揭穿了高于庄组岩溶热储,并揭露太古界厚度达1723.67m,给该地区岩溶热储下伏太古界的热流测定研究提供了条件。【研究方法】本文基于近稳态钻孔测温及岩心热导率测试,对D01井太古界进行了热流测定及分析。【研究结果】结果表明：D01井太古界呈显著的传导型地温特征,地温梯度为18.3℃/km,相比于新近系地温梯度48.6℃/km偏低。测得25块D01井太古界片麻岩岩心样品的热导率平均值为（2.41±0.40）W/(K·m)。根据钻孔测温数据及热导率测试,计算出D01井太古界2300～2700m深度的热流值为（44.1±7.0）mW/m²。同时,估算了D01井新近系400～800m深度段的热流值为84.6mW/m²,较太古界高出40.5mW/m²。【结论】分析认为D01井新近系较太古界高出热流主要为高孔渗岩溶白云岩层中地下水侧向热对流作用以及牛东断裂地下水垂向热对流作用共同所致。研究结果对前人提出的地下水运移聚热模式及导热断裂聚热模式提供了数据支撑,对雄安新区深部地热资源成因机制和太古界地温场研究具有重要意义。