共查询到20条相似文献,搜索用时 156 毫秒
1.
2.
通过对1:50 000嘉禾—塘村墟幅溪流重砂异常检查,在石炭系桂阳组地层中发现了原生汞矿床。矿体呈似层状、透镜状,主要矿石矿物为辰砂、少量辉锑矿,人工重砂中见银汞齐。矿石含Hg0.0004~0.416%,Ag0.23~47.37ppm,伴生元素Se含量较高,达15~43ppm。矿化严格受石炭系桂阳组(相当于岩关组邵东段)深灰色厚层状细晶云岩、中厚层碎裂化灰质云岩及北西西向断裂控制。围岩蚀变简单,仅见白云石化、方解石化及微弱的硅化。整个汞矿化带的分布受区域性近南北向断层控制。在该区1:200 000重砂扫面中圈定了很多辰砂异常,对这些异常进行进一步检查有可能发现新矿体。 相似文献
3.
4.
在前寒武纪变质岩区开展黄金异常查证的工作中,摸索出一套实用,快捷的综合重砂找金方法,工作过程为河流重砂加密缩小靶区,坡积重砂及简易人工重砂追索矿化蚀变带或矿(化)体风化露头,地表踏勘检查及简易人工重砂鉴定初步圈定矿(化)体,山地工程揭露与评价4个阶段。 相似文献
5.
福建西南部长汀、上杭一带广泛发育一套海相砂、泥质及硅质沉积的浅变质岩系,经过1:25万瑞金市幅区域地质调查,在证实“丁屋岭砾岩”的时代为晚泥盆世而从浅变质岩系中划分出去后,笔者将整合于早-中寒武世林田组之下的浅变质岩系,自下而上划分为姜畲坑组、赖坑组、南岩组和黄连组。 相似文献
6.
本文系第九分队罗璋同志根据工作中的实际经验所写。文中关于砂咀取样及砂碟与矿层交界处取样以及取样深度等问题,我们认为很有意义,可供同志们在工作中参考;如有不同的看法可以提出意见,共同讨论。 关于重砂取样问题在伊齐克松所著‘地质测量与概要普查时的重砂取样’里已有详细的叙述,但在一些实际问题上并非每个与重砂取样有关地质人员或其他工作人员的看法都是一 相似文献
7.
饶阳凹陷新近系馆陶组物源方向分析 总被引:2,自引:0,他引:2
张立强 《吉林大学学报(地球科学版)》2012,42(2):321-326,334
为了深入认识沉积物源的位置及古流向,通过矿物成分、岩屑特征、重矿物组合及分布、砂体展布特征等分析,对饶阳凹陷馆陶组的物源方向进行了系统研究。结果表明,饶阳凹陷新近系馆陶组沉积时期,盆地存在4个相对独立的物源及古水流体系:分别为来源于北或北东部物源自北向南或北东—南西流向的水系,来源于西部物源、西南—北东向展布的水系,源于西部物源、东西向展布的水系,源于南部或西南部物源、西南—北东向展布的水系。新近系的河流流向以南北向、沿盆地长轴方向为主,盆地内砂体具有南北向带状展布的特征;中部留路地区距离物源区相对较远、盖层较发育、储盖组合条件好,为饶阳凹陷新近系油气聚集的有利区带。 相似文献
8.
9.
10.
11.
12.
We apply a population synthesis technique to study the formation and evolution of low-mass X-ray binaries with black holes, observed as X-ray novae, from hierarchical triple systems. A scenario is suggested in which an inner close binary system evolves into an X-ray system with a large mass ratio. The high rate of accretion onto the neutron star leads to a common envelope stage, which may result in the formation of a Thorne-Zytkow (TZ) object. During its evolution, the envelope of the TZ object expands, encompassing the third star. The recurrent common-envelope stage decreases the size of the orbit of the third star, leading to the formation of a lowmass X-ray nova with a black hole. The dynamical stability of triple systems automatically ensures that only lowmass X-ray novae form. We also consider the possible formation of an X-ray nova from a binary in the case of asymmetrical core collapse during a supernova explosion. 相似文献
13.
冰点下水合物在多孔介质的生成是一个复杂的多相转化过程,为了研究冰点下多孔介质中水合物生成过程的水相转化率、气体消耗量与稳定压力等生成特性,在定容条件下,进行不同孔径与粒径的多孔介质中甲烷水合物在冰点下的生成实验。所使用的多孔介质平均孔径为1295 nm、1796 nm和3320 nm。研究结果表明:水合物生成结束时水的转化率随着初始生成压力的增大而增大,随着温度的升高而降低,随着孔径的增大而增大;在相同的孔径下,多孔介质粒径的增大降低了水合物的生成速率但对最终气体消耗量没有影响;在相同的温度下,随着初始生成压力的增大,实验最终压力、气体消耗量与最终水的转化率均随之升高;温度越高,不同的生成初始生成压力下体系的最终稳定压力与水的转化率相差越大;在多孔介质的毛细管作用力与结合水的共同作用下,冰点下水合物生成的水的转化率会大大地降低。在本实验条件下,水相转化为水合物的比例最高为32.39%。 相似文献
14.
沁水盆地煤层割理的充填特征及形成过程 总被引:3,自引:0,他引:3
煤层作为煤层气的源岩和储集层,与常规天然气储层不同在于煤储层是一种双孔隙岩层,由基质孔隙和裂隙组成,且有自身独特的割理系统,基质孔隙和割理的大小、形态、孔隙度和连通性等决定了煤层气的储集、运移和产出,其中以割理系统对煤层气的产出最为重要。本文以沁水煤田为例,对煤层割理、割理填充物类型、充填方式、自生矿物形成时代进行了研究,总结了填充物形成的先后顺序,并根据填充物的形成时代、煤层埋藏史等提出了割理形成的3种机制:埋藏增压机制;岩浆诱发机制;抬升卸压机制。 相似文献
15.
在总结分析前期钻井经验的基础上,从地质因素、钻井复杂情况、岩石可钻性、地层温度、钻井液密度、井身结构等方面分析了目前影响元坝区块深井钻井速度提高的因素。指出井身结构层次有限,不能完全有效封隔不同压力体系的地层以及须家河组地层可钻性差、埋深较深、段长,不能利用空气钻进行钻进是影响机械钻速的2个最重要原因。提出了气体钻井方案、钻头选型方案、进口动力钻具配合高效钻头钻须家河地层方案,以及采用特种井眼尺寸井身结构方案,为元坝区块深井钻井提供技术支持。 相似文献
16.
Organic material in meteorites provides insight into the cosmochemistry of the early solar system. The distribution of polycyclic aromatic hydrocarbons (PAHs) in the Allende and Murchison carbonaceous chondrites was investigated by use of a technique called microprobe laser-desorption laser-ionization mass spectrometry, which permits spatial resolution with approximately a 40-μm spot size. Sharp chemical gradients of PAHs are associated with specific meteorite features. The ratios of various PAH intensities relative to the smallest PAH, naphthalene, are nearly constant across the sample. These findings suggest a common origin for PAHs dating before or during the formation of the parent body, consistent with proposed interstellar formation mechanisms. 相似文献
17.
通过对钻探过程中井漏的复杂地质因素分析,提出了水化膨胀复合材料体系,并对该体系进行了膨胀性、封堵性及复合桥接堵漏模拟实验。实验结果表明,堵漏材料PAR具有很强的吸水膨胀性能,可膨胀至原体积的几十倍,且时间快有利于形成快速的封堵。材料PAR与稻谷和锯末形成的复合堵漏材料具有很强的堵塞率,可达70%以上。承压堵漏测量装置中测试表明:复合堵漏体系不仅能形成封堵,而且能够承受一定的压差。在云南临仓市勐简乡铅锌矿钻探过程中,运用复合堵漏体系满足了该地区复杂地矿钻探需要。 相似文献
18.
宝岛-长昌凹陷陵水组砂岩储集体目前是琼东南盆地油气勘探的重点目标.本文综合铸体薄片、激光粒度、元素地球化学、X衍射、扫描电镜、流体包裹体以及电子探针分析,探究宝岛凹陷北坡与长昌凹陷陵水组砂岩储层的成岩演化差异性.宝岛凹陷北坡的砂岩储层具有“粒度粗、稳定组分高”的强水动力特征,是海南岛物源体系下的三角洲沉积;而长昌凹陷砂岩储层具有“粒级偏细、泥质杂基重”的弱水动力特点,是神狐隆起、西沙隆起物源体系下的海底扇沉积.机械压实导致宝岛凹陷北坡的陵水组砂岩储层颗粒普遍呈现线状或凹凸接触.高热流背景导致长昌凹陷陵水组砂岩在海底以下浅埋条件(海底以下约1 400 m)下即可进入化学压实阶段,颗粒呈点-线接触,并伴生重晶石、片钠铝石等热液矿物.宝岛凹陷北坡存在早、晚两期烃类充注(14.5~10.0 Ma、2~0 Ma),期间被一期CO2充注分隔(7~3 Ma).长昌凹陷仅发育早期烃类充注(14.5~6.0 Ma),以及随后的一期CO2充注(5~0 Ma).陵水组砂岩储层演化在宝岛凹陷北坡总体以“海底以下缓慢深埋、缓慢升温”,天然气充注促进溶蚀和抑制胶结为特点,而长昌凹陷则以“海底以下浅埋、快速升温”,CO2持续充注促使碳酸盐或粘土或热液矿物胶结为特点. 相似文献
19.
Chondrule formation appears to have been a major event in the early solar system, but chondrule properties do not allow us to distinguish between several possible formation mechanisms. The physical nature of the precursors, especially grain size, must affect the textures of the chondrules they yield when heated. We melted precursors of different grain sizes, including extremely fine-grained crystalline aggregates analogous to nebular condensates, to see whether objects resembling most natural chondrules can be crystallized. With one-minute heating and moderate cooling rates, the grain size of the charges depends directly on the grain size of the starting material, for temperatures up to very close to the liquidus temperature. A single rapid heating of condensate-like material thus produces very fine-grained chondrules, like dark-zoned chondrules, for a very wide range of peak temperatures. It is incapable of generating the observed textural distribution of chondrules, which are predominantly porphyritic. The simplest model for chondrules, a single heating of unmodified condensate material, therefore appears unrealistic. Coarse-grained chondrules might be formed from fine-grained precursors by extended heating with evaporation leading to coarsening, or by multiple reheating events, with higher temperatures in subsequent events. Otherwise an origin from annealed condensates, planetary rocks, or by condensation of liquid and crystals is required. 相似文献
20.
The structure of a circumstellar envelope around a young binary T Tauri star is considered. The supersonic orbital motion
of the system components in the envelope gas leads to the formation of bow shocks around the star. Two- and three-dimensional
numerical modeling indicates an important role of these shocks in the formation of the structure of the circumbinary envelope.
In particular, for systems with circular orbits, the size of the central region of the envelope that is not filled with matter
(the “gap”) is essentially determined by the parameters of the bow shocks. These modeling results are supported by comparisons
of the obtained estimates for the gap parameters with observations. 相似文献