四川宣汉地区二叠系硅岩地球化学特征及成因研究   总被引：3，自引：1，他引：2       下载免费PDF全文

周新平  何幼斌  杜红权  李华 《古地理学报》2009,11(6):670-680

四川宣汉地区二叠系茅口组和吴家坪组的硅岩,主要以结核状、条带状和团块状产出。根据硅岩的岩石学及地球化学特征,对其成因进行了系统研究。野外观察硅岩形态多样,与围岩呈缝合线状接触,在剖面上受一定层位控制,团块状硅岩中含石灰岩斑块等。显微镜下观察,硅岩中见方解石残余结构及白云石菱形假晶等。野外观察和显微镜下观察表明这些硅岩应为交代作用形成。常量元素分析表明硅岩以SiO₂为主（69.61％～99.21％）,其他化学成分含量较低（0.01％～16.07％）,Fe/Ti、（Fe+Mn）/Ti及Al/（Al+Fe+Mn）值反映了硅岩的形成与热水活动有关,样品点在Al-Fe-Mn三角图中的投影位于富铁端;微量元素Co/Ni、V、Ti/V、Th/U和Rb/Sr值都较低,样品点在（Cu+Co+Ni）-Fe-Mn三角图中的投影也位于富铁端;硅岩中稀土元素总量低（低于10×10^-6）,Ce明显负异常,Eu弱负异常,LREE/HREE值低,Eu/Eu^*值相对较高。上述特征表明研究区硅岩在形成过程中有热水物质参与沉积,在成岩过程中通过SiO₂交代作用形成。  相似文献   

西北干旱地区大气降水δ18O的特征及水汽来源   总被引：7，自引：1，他引：6  

柳鉴容  宋献方  孙晓敏  袁国富  刘鑫  王仕琴 《地理学报(英文版)》2009,19(2):164-174

In order to reveal the characteristics and climatic controls on the stable isotopic composition of precipitation over Arid Northwestern China, eight stations have been selected from Chinese Network of Isotopes in Precipitation (CHNIP). During the year 2005 and 2006, monthly precipitation samples have been collected and analyzed for the composition of δD and δ18O. The established local meteoric water line δD=7.42 δ18O+1.38, based on the 95 ob-tained monthly composite samples, could be treated as isotopic input function across the region. The deviations of slope and intercept from the Global Meteoric Water Line indicated the specific regional meteorological conditions. The monthly δ18O values were characterized by a positive correlation with surface air temperature (δ18O (‰) =0.33 T (℃)-13.12). The amount effect visualized during summer period (δ18O (‰) = -0.04P (mm)-3.44) though not appeared at a whole yearly-scale. Spatial distributions of δ18O have properly portrayed the atmospheric circulation background in each month over Arid Northwestern China. The quan-titative simulation of δ18O, which involved a Rayleigh fractionation and a kinetic fractionation, demonstrated that the latter one was the dominating function of condensation of raindrops. Furthermore, the raindrop suffered a re-evaporation during falling processes, and the pre-cipitation vapor might have been mixed with a quantity of local recycled water vapor. Multiple linear regression equations and a δ18O-T relation have been gained by using meteorological parameters and δ18O data to evaluate physical controls on the long-term data. The estab-lished δ18O-T relation, which has been based on the present-day precipitation, could be considered as a first step of quantitatively reconstructing the historical environmental climate.  相似文献   

山东省平邑归来庄金矿深部矿床特征及成矿规律研究          下载免费PDF全文

张国权 《山东国土资源》2017,33(9):7-13

山东平邑归来庄金矿深部矿床,受近EW向归来庄F_1断裂和中生代隐爆角砾岩体共同控制,赋存于Ⅰ号构造蚀变带内,属"中低温热液隐爆角砾岩型"。通过对矿床地质特征、矿体特征、矿石质量、矿石类型、围岩蚀变、找矿标志及矿床成因等方面的研究,总结了该区基本成矿规律:归来庄F_1断裂为一经历多次活动的构造隐爆角砾岩蚀变带,既控矿又赋矿,矿体的展布、金的富集与隐爆角砾岩体关系密切;矿体总体向南西侧伏,具有侧伏向延伸大于倾向延长的特点,侧伏向深部仍可能再次出现富集带,具有良好的找矿前景和一定的资源潜力。  相似文献   

山东枣庄杨家堡子铁矿床地质特征及成因探讨          下载免费PDF全文

张桂林  邵爱东  张伟 《山东国土资源》2017,33(9):19-25

杨家堡子铁矿位于山东省枣庄市峄城区峨山镇,隶属苍峄铁成矿带,矿体赋存于新太古代泰山岩群山草峪组上部的变质岩中。该矿床内圈定磁铁矿体11个,求得铁矿石(333)资源量3 378.2万t,矿床平均品位TFe 33.30%,mFe 22.64%。主矿体为Ⅲ-6矿体,占矿床总资源量的83.69%,其长度1 137 m,最大斜深1 065 m,埋深707~1 369m,形态复杂程度中等,品位变化属均匀类型。含矿岩石为磁铁石英角闪岩。矿石中的主要有用组分为Fe,伴生元素含量较低,均无综合回收利用价值,有害组分S、P的含量均较低,经选矿后可达到炼钢及炼铁要求。矿石结构主要有粒状变晶结构和柱状变晶结构;矿石的构造主要为条带状构造,块状构造的矿石较少,但品位相对较高。矿石自然类型为原生磁铁矿石,工业类型属需选磁性铁矿石。该矿床成因与苍峄铁矿一脉相承,为典型的BIF型铁矿。根据区内以及邻区的见矿情况结合磁异常特征分析,杨家堡子矿区有良好的找矿前景。  相似文献   

华庆地区长63段低渗储层特征及优质储层主控因素     

李福来  王石头  苗顺德  杨军侠  徐志尧  李文帅 《吉林大学学报(地球科学版)》2015,45(6):1580-1588

综合运用岩心观察、薄片鉴定、物性分析、压汞分析及试油分析等技术方法,对华庆地区长6₃段低渗储层特征进行了系统研究,分析了低渗储层的成因,并探讨了优质储层的主控因素。结果表明,华庆地区长6₃段储层的厚层块状砂岩主要由具有液化流性质的砂质碎屑流沉积形成的相对较厚块状砂岩纵向叠置组成。岩石类型主要为长石砂岩,其次为岩屑长石砂岩;储层具有低孔特低孔-特低渗透超低渗透特征;储集空间主要包括粒间原生孔隙、次生溶蚀孔隙及晶间微孔隙,为小孔微细喉型孔隙结构。杂基含量高、成分成熟度和结构成熟度差是华庆地区长6₃低渗储层形成的主控因素,压实作用对其形成起到强化作用。沉积鼎盛时期水动力强的主力沉积期次,形成泥质含量较低的砂岩是优质储层形成的主控因素,而较大的储层厚度是优质储层形成的必要条件。  相似文献   

IRCS/Subaru observations of water in the inner coma of Comet 73P-B/Schwassmann-Wachmann 3: Spatially resolved rotational temperatures and ortho-para ratios     

Boncho P. Bonev  Michael J. Mumma  Hitomi Kobayashi 《Icarus》2008,196(1):241-248

Comet 73P-B/Schwassmann-Wachmann 3 was observed with IRCS/Subaru at geocentric distance of 0.074 AU on UT 10 May 2006. Multiple H₂O emission lines were detected in non-resonant fluorescence near 2.9 μm. No significant variation in total H₂O production rate was found during the (3 h) duration of our observations. H₂O rotational temperatures and ortho-to-para abundance ratios were measured for several positions in the coma. The temperatures extracted from two different time intervals show very similar spatial distributions. For both, the rotational temperature decreased from ∼110 to ∼90 K as the projected distance from the nucleus increased from ∼5 to ∼30 km. We see no evidence for OPR change in the coma. The H₂O ortho-para ratio is consistent with the statistical equilibrium value (3.0) for all spatially resolved measurements. This implies a nuclear spin temperature higher than ∼45 K.  相似文献   

Rebuttal to “Comment on the paper “Comparison of the composition of the Tempel 1 ejecta to the dust in Comet C/Hale-Bopp 1995 O1 and YSO HD 100546” by C.M. Lisse, K.E. Kraemer, J.A. Nuth III, A. Li, and D. Joswiak"     

C.M. Lisse 《Icarus》2008,195(2):941-944

This response is to address the comments made by Drs. J. Crovisier and D. Bockelee-Morvan concerning the spectral analysis of Lisse et al. [Lisse, C.M., Kraemer, K.E., Nuth, J.A., Li, A., Joswiak, D., 2007. Icarus 187, 69-86] of the mid-IR ISO SWS spectrum of Comet Hale-Bopp 1995 O1 taken on October 6, 1996, and to support the conclusions made in Lisse et al. concerning the positive detection of PAHs in this comet. We also present some additional information determined from the Deep Impact and STARDUST missions, demonstrating the presence of PAHs in other comets, to support the plausibility of the Hale-Bopp PAH detection.  相似文献   

鄂尔多斯盆地NX地区长6段特低-超低渗储层特征及其成因          下载免费PDF全文

黄春梅  钟红利  闫凤平  蒋司淋  白二林  张凤奇  武富礼  刘伟 《沉积与特提斯地质》2019,39(4):38-46

根据物性测试、铸体薄片、扫描电镜、X射线衍射、压汞等资料,对鄂尔多斯盆地NX地区长6段储层特征及成因进行了研究。结果表明,研究区长6段砂岩储层为低孔-特低、超低渗透储层,主要孔隙类型为残余粒间孔和次生溶蚀孔,孔喉组合主要为中孔-细喉型和小孔-细喉型。早期的压实作用、胶结作用是使研究区长6段储层物性变差的两个重要作用。压实作用丧失的孔隙占原始孔隙的45.9%～65.6%,平均为56.5%;胶结作用丧失的孔隙占原始孔隙的21.8%～46.4%,平均为28.3%,粘土矿物、碳酸盐是造成物性降低的主要胶结物类型。长石、浊沸石、岩屑等的溶蚀作用极大改善了储层物性,改善了现今孔隙的22.2%～71.4%,平均44.2%。早白垩世末期,研究区长6储层已基本变为特低～超低渗透,该时期之后,成岩作用对储层物性影响较弱,储层物性基本保持到现今。  相似文献   

Rare Earth Elements Composition and Constraint on the Genesis of the Polymetallic Crusts and Nodules in the South China Sea     

GUAN Yao  SUN Xiaoming  SHI Guiyong  JIANG Xiaodong  LU Hongfeng 《《地质学报》英文版》2017,91(5):1751-1766

The rare earth elements(REE) composition of the polymetallic crusts and nodules obtained from the South China Sea(SCS) were analyzed through inductively coupled plasma mass spectrometry.Results revealed great differences in the REE abundances(∑REE) of the SCS polymetallic crusts and nodules; the crusts show the highest ∑REE, whereas the nodules exhibit the lowest ∑REE. The similarity in their NASC-normalized patterns, the enriched light REE(LREE), the markedly positive Ce anomaly(δCe), and the non-or weakly positive Eu anomaly(δEu), suggest that the polymetallic crusts and nodules are of hydrogenetic origin. Moreover, the REE contents and their relevant parameters are quite different among the various layers of the crusts and nodules, which probably results from the different marginal sea environments and mineral assemblages of the samples. The growth profiles of the SCS polymetallic crusts and nodules reveal the tendency ∑REE and δCe to slightly increase from the outer to the inner layers, suggesting that the growth environments of these samples changed smoothly from an oxidizing to a relatively reducing environment; in addition, the crust ST1 may have experienced a regressive event(sea-level change) during its growth, although the REE composition of the seawater remained relatively stable. On the basis of the regional ∑REE distribution in the SCS crusts and nodules,the samples collected near the northern margin were influenced by terrigenous material more strongly compared with the other samples, and the REE contents are relatively low. Therefore, the special geotectonic environment is a significant factor influencing the abundance of elements, including REE and other trace elements. Compared with the oceanic seamount crusts and deep-sea nodules from other oceans,the SCS polymetallic crusts and nodules exhibit special REE compositions and shale-normalized patterns, implying that the samples are of marginal sea-type Fe-Mn sedimentary deposits, which are strongly affected by the epicontinental environment, and that they grew in a more oxidative seawater environment. This analysis indicates that the oxidized seawater environment and the special nano property of their Fe-Mn minerals enrich the REE adsorption.  相似文献   

鄂尔多斯盆地姬塬西部三叠系延长组长8油层组成岩作用与致密化过程^*          下载免费PDF全文

汪洋  刘洛夫  李树同  吉海涛  李林泽  罗泽华  许同 《古地理学报》2017,19(5):892-906

利用岩心、铸体薄片、扫描电镜、碳氧同位素及流体包裹体等资料,对鄂尔多斯盆地姬塬西部三叠系延长组长8油层组致密储集层特征进行了研究,重点分析了储集层成岩作用特征和储集层致密化成因机制及过程。研究区长8油层组砂岩主要为岩屑长石砂岩和长石岩屑砂岩,经历了压实—压溶、胶结、交代、溶蚀及构造破裂等成岩作用,整体处于中成岩A期晚期。典型成岩序列依次为机械压实、绿泥石黏土膜、早期(泥晶)方解石胶结、石英次生加大、长石、岩屑溶蚀、自生高岭石胶结、自生石英胶结、中期(含)铁方解石胶结。综合研究认为:(1)近物源伴随湖平面快速上升的沉积环境提供了储集层致密化的物质基础,不同沉积微相储集层物性差别较大,分流河道最好,分流间湾最差;(2)长8油层组原始孔隙度为41.35%,压实作用损孔率为50.67%,造成储集层孔隙度急剧降低,胶结作用损孔率为37.48%,导致孔隙度进一步减小,溶蚀作用仅增加了3.26%的孔隙度,难以有效改善储集层质量;(3)上述沉积与成岩因素共同导致储集层致密,致密化过程可分为压实孔隙骤减阶段、早期胶结减孔阶段、溶蚀作用增孔阶段和晚期胶结致密阶段共4个阶段;(4)油气大量充注期储集层孔隙度远低于10%,长8油层组先致密后成藏。  相似文献