民和盆地中侏罗统煤-油页岩层系生油特征   总被引：4，自引：0，他引：4  

王春江  王有孝 《沉积学报》1997,15(1):59-64

本文简要论述了民和盆地中侏罗统含煤及油页岩层系的生油特征，探讨了盆地独特的石油地质和地球化学条件。原油主要地化特征为:Ｐｒ/Ｐｈ比值偏高（２.６５-３.１５）、甾烷/藿烷比值极低（０.０３）、Ｃ_２７甾烷较丰富、Ｔｓ/Ｔｍ＞１低硫芴/氧芴比值、较高含量的Ｃ_２９降新藿烷及重排藿烷类化合物及相对丰富的长链联苯及烷基四氢萘系列化合物。中侏罗统煤－泥页岩层系含生油潜力明显不同的多类型油页岩，多数油页岩属由藻类和陆生高等植物母质组成的混合型有机质，沉积环境为淡水－微咸水弱氧化条件，其地化特征也表现为高Ｐｒ/Ｐｈ比值（平均为１。９８），低甾烷/藿烷及低硫芴/氧芴比值等特征。某些油页岩富含Ｃ_２９降新藿烷及重排藿烷系列化合物，它们应为主力源岩。油页岩多含再沉积型或沉积改造型有机质。异常地热作用对源岩演化及原油地化特征有重要影响。  相似文献   

孔隙流体压力与流体排驱的关系   总被引：2，自引：3，他引：2  

冯乔  张小莉 《地质论评》1997,43(3):297-302

本文讨论了在压实作用下孔隙流体压力的形成以及与流体排驱的关系，指出异常孔隙流体压力是因岩石渗透率变化引起毛细管力增加而产生的，且二者之间在流体压力孕育过程中一直维持一个动态平衡状态。对于连续沉积的盆地，只有当异常孔隙流体压力增加到超过岩石的抗剪强度时，因岩石发生剪切破裂导致毛细管力降低，流体才被排出；对于强烈构造变动的盆地，因地层大量剥蚀引起负荷压力降低，其降低幅度达到或超过岩石的抗张强度时，岩石  相似文献   

铜陵地区老鸦岭层状钼矿床铅同位素组成研究   总被引：1，自引：0，他引：1  

喻钢  陈江峰  钱卉  陈树榆  杨刚  闫峻  张成火 《矿床地质》2004,23(4):422-430

安徽铜陵老鸦岭矿床中二叠系大隆组(P2d)顶部的含矿(钼矿化)黑色页岩以及附近(立新煤矿)同一层位不含矿黑色页岩的实测铅同位素组成分别为：^206Pb/^204Pb20.20～22.37,^207Pb/^204Pb15.67～15.82,^208Pb/^204Pb38.47～38.60和^206Pb/204Pb18.83～20.80,^207Pb/^204Pb15.65～15.76,^208Pb/^204Pb38．84～39．22。对137Ma的放射成因Pb进行校正后的铅同位素组成表明，含矿黑色页岩和不含矿黑色页岩均与燕山晚期火成岩无关，老鸦岭含矿黑色页岩可能具沉积成因。对沉积(约250Ma)以来的放射成因Pb进行校正后的铅同位素组成表明：不含矿黑色页岩的Pb源自上地壳，而含矿黑色页岩的Pb(因而推测其他成矿金属)可能源于上地壳物质(与不含矿黑色页岩的Pb源相似)与下地壳物质的混合。  相似文献   

铂族元素的表生地球化学研究进展   总被引：2，自引：0，他引：2  

皮道会  邓海琳  李朝阳  朱维光 《矿物岩石地球化学通报》2004,23(4):355-361

基性-超基性岩及黑色页岩等风化过程中铂族元素发生了活化和迁移。铂族元素在岩体附近土壤、植物和水体等表生介质中的迁移富集特征可以用来寻找岩浆型铂族元素矿床。黑色页岩风化过程中，Os的表生迁移对海洋^187Os／^188Os值上升有重要意义。此外，作为重金属元素，机动车铂族元素催化剂在环境中的释放，也会带来潜在的生态环境和人体健康问题。  相似文献   

宁夏中卫县沙坡头地区黑色泥质页岩固沙性能研究     

郭进京  杜东菊  韩文峰  杨爱武 《中国地质灾害与防治学报》2004,15(1):121-123,133

我国西北干旱半干旱地区，生态环境极为脆弱，土地沙漠化问题十分突出。防风固沙，恢复植被，遏制沙漠化，改善生态环境，是我国西部大开发战略和加快西部经济腾飞的主要任务之一。防风治沙首先要解决的问题是固沙保水。文章提出了利用宁夏腾格里沙漠东南缘中卫县沙坡头地区香山北麓的黑色泥质页岩在自然条件下天然胶结成壳作用于固沙的可能性。这类黑色泥质页岩具有遇水则吸水软化，风干则形成薄硬壳之特点。在斜坡坡面上或坡脚风化破碎或构造破碎或人工开挖的黑色泥质页岩碎块堆积的表面常形成1层1～5cm的硬壳。这类黑色泥质页岩在500℃时灼减量高达17．56％，说明具有很高的有机质含量，同时P2O5，和K2O含量也较高，有利于成壤和植物生长。黑色泥质页岩的天然胶结成壳作用与地表破碎的黑色泥质页岩堆积和特定的干旱半干旱气候以及本身成分、结构有关。这一硬壳层不但具有一定的强度和抗风蚀能力，而且还具有一定的吸水性和保水性。因此，借鉴草方格固沙方法，就地取材，充分利用黑色泥质页岩在自然条件下的天然胶结成壳性能，用于沙漠治理中的固沙。进一步对黑色泥质页岩天然胶结成壳的机理进行深入研究，并开展黑色泥质页岩固沙试验研究，有可能为腾格里沙漠治理开辟新的途径。  相似文献   

Microthermometric measurement of fluid inclusions and its constraints on genesis of PGE-polymetallic deposits in Lower Cambrian black rock series, southern China   总被引：2，自引：0，他引：2  

WANG Min 《中国地球化学学报》2005,24(4):297-305

Systematic microthermometric measurements of fluid inclusions in the PGE-polymetallic deposits hosted in the Lower Cambrian black rock series in southern China were performed, and the results suggest: (1) there exist two types of fluid inclusions. TypeⅠis of NaCl-H2O system with low-medium salinity, and its homogenization temperatures (Th) and salinities are 106.9- 286.4℃ and ( 0.8- 21.8) wt%NaCl eq. respectively; TypeⅡ is of CaCl2-NaCl-H2O system with medium-high salinities, and its homogenization temperatures and salinities range from 120.1℃ to 269.6℃ and ( 11.4- 31.4) wt%NaCl eq., respectively. The typeⅡ fluid inclusions have been discovered for the first time in this kind of deposits; (2) two generations of ore-forming fluids were recognized. Characteristics of fluid inclusions in the PGE-polymetallic ores and carbonate-quartz stockworks in the underlying phosphorites are almost of no difference, they may represent ore-forming fluids at the main metallogenic stage. The peak value of homogenization temperature of those fluid inclusions is about 170℃, while their salinities possess a remarkable bimodal distribution pattern with two peak values of (27-31) wt%NaCl eq. and (4-6) wt%NaCl eq. On the contrary, fluid inclusions in the carbonate-quartz veins in the hanging wall may represent ore-forming fluids at the post-metallogenetic stage. The homogenization temperatures and the peak values of salinities are mostly 130-170℃ and (12-14) wt%NaCl eq., respectively; (3) nobel gas isotopic composition analyses in combination with the microthermometric measurements of fluid inclusions suggest that the ore-forming fluids at the main metallogenetic stage were probably derived from mixing of basinal hot brines with the CaCl2-NaCl-H2O system and seawater with the NaCl-H2O system; (4) in the Early Cambrian, the basinal hot brines were trapped in the Caledonian basins, which were distributed along the southern margin of the Yangtze Craton, and where giant thick sediments were accumulated, and expelled and migrated laterally along the strata because of the pressure caused by overlying sediments. The basinal hot brines absorbed Ni, Mo, V, PGE from the surrounding rocks and were transformed into ore-bearing hydrothermal fluids with the CaCl2-NaCl-H2O system and medium-high salinities, then ascended along faults and mixed with seawater of the NaCl-H2O system, and finally PGE-polymetallic deposits or occurrences were formed in the black rock series.  相似文献   

小动力旋挖钻机用嵌岩短螺旋钻头结构形式的改进          下载免费PDF全文

刘南昌  胡继良  黄玉文  翁炜  张宏智 《探矿工程》2005,32(2):43-43,46

采用小动力无加压旋挖钻机在粒径较大的卵砾石地层和泥页岩地层中进行1500 mm以上大口径钻孔灌注桩施工，由于钻机动力小且不能加压，用常规嵌岩短螺旋钻头钻进出现进尺慢或不进尺现象。通过对河南西峡县宛西制药责任有限公司新厂房桩孔施工过程中出现此种现象的分析和处理，提出了嵌岩短螺旋钻头针对性的改进措施，并取得了良好效果。  相似文献   

GRB 170817A的洛伦兹因子和观测角          下载免费PDF全文

林一清 《天文学报》2020,61(1):6

伴随着引力波事件GW170817的短暴GRB (Gamma-Ray Burst) 170817A首次提供了双中子星并合与短暴相联系的直接证据.但是短暴GRB 170817A具有非常弱的光度,意味着观测的视线方向可能偏离喷流轴方向.根据短暴静止系的峰值能量E_(p,i)和各向同性光度L_(iso)。之间的关系以及洛伦兹因子Γ和L_(iso)。之间的关系估算了短暴GRB 170817A以及长短暴GRB 060614观测角与喷流边缘的夹角θ'_(obs)和洛伦兹因子Γ,结果表明GRB 170817A的Γ=45±27,θ'_(obs)=2.2±0.5°,而GRB 060614的Γ=214±93,θ'_(obs)=0.5±0.1°.这个结果相当于GRB 170817A的正轴各向同性光度L_(iso,on)=(2.1±0.7)×10~(49) erg·s~(-1),比典型的短暴少2-3个数量级.GRB 060614的L_(iso,on)=(5.12±1.91)×10~(51) erg·s~(-1)与典型短暴相当.这意味着GRB 060614可能属于短暴类型,而GRB 170817A可能本质上就是一个弱暴.  相似文献   

Spatial and temporal variations of albedo on nine glaciers in western China from 2000 to 2011          下载免费PDF全文

Jie Wang  Baisheng Ye  Yuhuan Cui  Xiaobo He  Guojing Yang 《水文研究》2014,28(9):3454-3465

This research demonstrates the spatiotemporal variations of albedo on nine glaciers in western China during 2000–2011, by the albedo derived from two types of datasets: Landsat TM/ETM + images and MOD10A1 product. Then, the influence factors of glacier albedo and its relationship with glacier mass balance are also analyzed by the correlation approach, which is frequently used in geostatistics. The paper finds that there are different spatiotemporal variations over the glaciers in western China: (1) For a single glacier, the albedo varies gently with altitude on its tongue and increases fast in the middle part, while in the accumulation zones, the albedo value appears in the form of fluctuation. This could provide a quantitative method to retrieve the snowline by determining the threshold albedo value of snowpack and bare ice. (2) For the glaciers in western China, the albedo decreases with distance to the center of Tibetan Plateau (TP). This may relate to the elevation of glacier, for the speed of glacier retreat highly depends on air temperature. (3) In the summer period, albedo on most glaciers declines over the last 12 years, and it decreases much faster in southeastern TP than other regions, for which air temperature overwhelms the black carbon concentration. In addition, the trend of glacier albedo in summer is greatly correlated with that of measured glacier mass balance, which implies that the long‐term albedo datasets by remote sensing technology could be used to monitor and predict the change of glacier mass balance in the future. Copyright © 2013 John Wiley & Sons, Ltd.  相似文献   

Evidence for the Retrograde Accretion onto Supermassive Black Holestwo     

Wang Kai  Huang Zheng-peng  Wang Jian-min 《Chinese Astronomy and Astrophysics》2019,43(2):217-224

Recently, Sloan Digital Sky Survey successfully carried out the reverberation mapping of a sky area, aiming to test the R ? L relation that has been already widely used. Here, R is the responsivity-weighted radius of the broad line region, and L is the optical luminosity at 5100 Å. Two results have been obtained from the data in the first year: (1) The time lags of AGNs (Active Galactic Nuclei) with a high accretion rate are much shorter than that estimated from the R ? L relation, which confirmed the results of reverberation mapping observations made by the Lijiang 2.4 meter telescope. (2) Some AGNs with a lower accretion rate also have very short time lags. The shortening of the time lags of the AGNs with a low accretion rate is caused by the retrograde accretion of black holes. This result has verified from observations the theoretical prediction made by Wang et al. (2014). The discovery of the black holes with a retrograde accretion has important significance, it indicates that the cosmological evolution of the black holes in quasars is implemented via the inherently random accretion.  相似文献