Differences in animal ¹³C, ¹⁵N and D abundance between a polluted and an unpolluted coastal site: Likely indicators of sewage uptake by a marine food web     

G.H. Rau  R.E. Sweeney  I.R. Kaplan  A.J. Mearns  D.R. Young 《Estuarine, Coastal and Shelf Science》1981,13(6):701-707

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新疆西准噶尔表壳元素地球化学特征的地质意义     

夏希凡  汪洋  杜佩轩 《新疆地质》2006,24(4):392-394

根据西准噶尔地区1∶20万化探均匀采集的780余个岩石样品分析结果,基于全样本统计和迭代剔除方法,得到新疆西准噶尔地区表壳(出露地壳)的36种元素丰度值.同时对其中的SiO2、TiO2、Al2O3、TFe2O3、MgO、MnO、CaO、Na2O、K2O、P2O5 10种常量元素氧化物,按氧化物之和为100%进行了归算.西准噶尔地区表壳在化学成份上相当于花岗闪长岩.与日本岛弧上地壳元素丰度值相比,西准噶尔地区表壳富集TFe2O3、Na2O、TiO2、P2O5和Cu、Sr,而亏损CaO和Co、Cr、Nb、Ni、Pb、Sb、Th等元素.从元素比值来看,西准噶尔地区表壳的K/La、K/Th、Nb/La、Th/La、La/As、La/Sb等比值与日本岛弧上地壳相应元素比值相当;而K/Na比值低于岛弧上地壳,La/Cr比值高于岛弧上地壳.西准噶尔地区表壳在成分特征上与典型的岛弧造山带上地壳相近.加里东期和海西期岛弧造山作用是影响和制约西准噶尔地区表壳元素地球化学特征的重要地质因素.  相似文献   

中国海相碳酸盐岩评价中有关有机质丰度下限的几点讨论     

刘华  彭平安  刘大永  林玉祥 《地质通报》2006,(Z2)

综述了中国海相碳酸盐岩有机质下限研究的若干进展,认为针对不同需求,应提出碳酸盐岩烃源岩最低下限、有效烃源岩下限、战略选区下限3个不同的下限标准。高成熟碳酸盐岩原始有机质丰度恢复一直存在争议,根据生烃动力学,结合热史,可实现原始有机质总量的恢复。碳酸盐岩中泥质与有机质丰度、排烃能力是否相关仍存在争论,认为碳酸盐岩中泥质的作用仍有待进一步研究。  相似文献   

云南澜沧江中南段多金属成矿谱系分析     

陈守余  赵鹏大  胡光道 《地质找矿论丛》2007,22(3):172-178

基于GIS空间分析技术,对云南澜沧江中南段多金属矿床的赋矿地层时间谱系、容矿构造空间谱系和矿床成因谱系进行了较系统的分析.研究表明,下-中元古界、三叠系、泥盆系、二叠系是本区最重要的赋矿层位,有两个聚矿期和多个时代地层含矿的特点,不同时代地层的含矿性具有多样性和专属型特征,元古宙火山沉积为主的建造是铁-铜、钨-锡矿为主的赋矿层位,晚古生代-中生代早期是沉积、裂谷火山活动强烈时期,金、铜、铅、锌、银、汞、锑、钨、锡多金属矿床高度聚集.自东向西为中生代坳陷区金、铜、镍成矿带,思茅-龙洞河晚古生代-三叠纪沉积盆地铜、铅、锌、银成矿带,岩浆弧地块钨、锡、铅-锌、铁成矿带,浅变质岩基底铅-锌-银、铁成矿带,被动边缘活动带金、铅-锌-银、锡成矿区和保山-镇康微地块铅-锌、铜、铁、汞成矿带,构成了容矿构造空间谱系.全区多金属矿床有沉积、沉积改造、岩浆-变质热液、火山沉积-火山热液四大成矿谱系,14种成矿类型,铜多金属、铅-锌-银、锡-钨矿床是研究区最具找矿前景的优势矿种.  相似文献   

金矿的地质地球化学找矿标志     

薛水根 《江苏地质》2007,31(1):7-9

地层和岩浆岩含金高丰度是金矿赋集的物质来源,断裂构造是容矿、储矿的空间。一般说来,金成矿物质越丰富,就越有利于形成大矿、富矿。以江西金矿找矿为例,阐述正确圈定金异常,合理布置探矿工程,获得找金成果新突破的实际意义。  相似文献   

Comparison of element abundance between the exposed crust of the continent of China and the global averaged upper continental crust: Constraints on crustal evolution and some speculations     

Wang Yang 《Frontiers of Earth Science》2007,1(1):69-79

Based on the results of a study of regional element abundance in eastern China and the 1:200 000 geochemical surveys in northern Xinjiang, the element geochemical characteristics of the exposed crust in 23 tectonic units of the continent of China are summarized. Compared with the global average abundance of the upper continental crust, the exposed crust of the continent of China is compositionally more evolved than the upper crust of the island arc, but less evolved than the mature Precambrian Canadian shield. The exposed crust of the North China and Yangtze platforms has a lower SiO₂ content, but markedly higher CaO and MgO contents due to the presence of widespread carbonate strata, which suggests that we should not neglect the contribution of carbonate rocks in the study of the exposed crust and the element abundance of the upper crust. In comparison with two recently published average compositional models of the global upper continental crust, the exposed crust of the continent of China is depleted in Au, Hg, Mo, Sn, and W, which suggests that their abundance in the present global models is overestimated. The exposed crust of the North China platform and the Qinling-Dabieshan fold belt to its south has lower μ(²³⁸U/²⁰⁴Pb) values (<8), but other regions of the continent of China exhibit much higher μ values, which implies that the low μ feature of the North China platform and its adjacent regions does not have global significance. Considering the apparent lateral variation in composition of the exposed crust for the tectonic units of the continent of China, there is no adequate reason to take the average upper crust compositional model of the North China platform and its adjacent regions as a reliable composition representative for Chinese and global upper continental crust composition. Translated from Geological Bulletin of China, 2005, 24(10–11): 906–915 [译自: 地质通报]  相似文献   

Methane Abundance on Titan, Measured by the Space Telescope Imaging Spectrograph     

Mark T. LemmonPeter H. Smith  Ralph D. Lorenz 《Icarus》2002,160(2):375-385

Although methane is the dominant absorber in Titan's reflection spectrum, the amount of methane in the atmosphere has only been determined to an order of magnitude. We analyzed spectra from the Space Telescope Imaging Spectrograph, looking at both a bright surface region (700-km radius) and a dark surface region. The difference between the spectra of the two regions is attributed to light that has scattered off the surface, and therefore made a round-trip through all of Titan's methane. Considering only absorption, the shape of the difference spectrum provides an upper limit on methane abundance of 3.5 km-am. Modeling the multiple scattering in the atmosphere further constrains the methane abundance to 2.63±0.17 km-am. In the absence of supersaturation and with a simplified methane vertical profile, this corresponds to a surface methane-mole fraction near 3.8% and a relative humidity of 0.32. With supersaturation near the tropopause, the surface methane mole fraction could be as low as 3%.  相似文献   

History of Star Formation and Chemical Enrichment in the Milky Way Disk   总被引：2，自引：0，他引：2  

Rui-Xiang Chang  Cheng-Gang Shu  Jin-Liang Hou Shanghai Astronomical Observatory  Chinese Academy of Sciences  Shanghai CAS-Peking University Joint Beijing Astronomical Center  Beijing 《中国天文和天体物理学报》2002,2(3)

Based on a physical treatment of the star formation law similar to that given by Efstathiou, we have improved our two-component chemical evolution model for the Milky Way disk. Two gas infall rates are compared, one exponential, one Gaussian. It is shown that the star formation law adopted in this paper depends more strongly on the gas surface density than that in Chang et al. It has large effects on the history of star formation and gas evolution of the whole disk. In the solar neighborhood, the history of chemical evolution and star formation is not sensitive to whether the infall rate is Gaussian or exponential. For the same infall time scale, both forms predict the same behavior for the current properties of the Galactic disk. The model predictions do depend on whether or not the infall time scale varies with the radius, but current available observations cannot decide which case is the more realistic. Our results also show that it would be inadequate to describe the gradient evolution along the Gala  相似文献   

Figure 1 Linear fitness of the index H' respectively calculated by the number or the area of the related Sus Pedodiversity analysis in Hainan Island     

ZHANG Xuelei  CHEN Jie  ZHANG Ganlin  TAN Manzhi  J.J. Ibá  ?ez 《地理学报》2003,13(2):181-186

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Verteilung und Wanderung von Neunaugen im Elbeästuar (Deutschland)     

Ralf Thiel  Volker Salewski 《Limnologica》2003,33(3):214-226

From March 1989 until May 1995 overall 675 hauls were performed using a commercial stow net vessel to get information concerning spatial and seasonal distribution, length frequency distribution, stock situation and migration patterns of lampreys in the Elbe estuary in northern Germany.2217 river lampreys (Lampetra fluviatilis) and 10 sea lampreys (Petromyzon marinus) were caught during the whole study period. The river lamprey occurred in 40.3% of the performed stow net hauls. The catch success was highest in the western main channel, whereas the frequency of occurrence of river lampreys was only about 10.9% at the most upstream site in the southern marginal area. In 1989 and 1990 significantly more than 50% of the hauls contained river lampreys. In contrast, from 1991 to 1995 their frequency of occurrence was lower than 40%, in 1991 even lower than 20%. Sea lampreys occurred only at 6 from 9 sampled sites and were only observed in 1990 and 1992-1994.Total lengths of river lampreys varied between 7 and 46 cm. Based on the length frequency distribution, the following three size classes of river lampreys were separated: LF I (7 to 16 cm), LF II (17-26 cm) and LF III (27-46 cm). The majority of the caught individuals could be grouped in size class LF III. Total lengths of sea lampreys ranged between 69 and 85 cm and were restricted to only one size class (PM III).70% of all sea lampreys were caught in April and May. Most of the sea lampreys were observed in the eastern main channel. The maximum average abundance of river lampreys was observed with 6.75 Ind · m⁻³ · 10⁻⁶ in the same area in 1992. However, in 1993 and 1994 the highest average abundances of river lampreys occurred in the western main channel.Based on redundance analysis, a significant correlation between the abundances of lampreys and the environmental variables autumn, spring, summer, salinity, water temperature, grain size, new moon and first moon quarter was found. The downstream migrating river lampreys of size class LF I und the sea lampreys during their anadromous spawning migration showed highest abundances mainly in spring, whereas high abundances of river lampreys of size class LF II in the feeding phase occurred in summer. The presence of both size classes LF I and LF II confirms the successful reproduction of river lampreys in the catchment area of the Elbe. The observation of river lampreys of size class LF III during their anadromous spawning migration was closely correlated with the variable autumn. A spring spawning migration of river lampreys was not observed.  相似文献