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1.
陕西渭河盆地固市凹陷渭热2井组 甲烷气成因及其意义   总被引:1,自引:0,他引:1  
李玉宏  王行运  韩伟  宫振奇 《地质通报》2013,32(11):1790-1797
渭河盆地固市凹陷渭热2井组甲烷气的成功点火,再一次引起人们对渭河盆地油气资源前景的关注。渭热2井组及邻区7口井天然气组分、甲烷C同位素等分析指标显示,该区甲烷气具有2种成因类型,浅部气层为新近系张家坡组生物成因气,中深部天然气来自前新生界煤型热解-裂解气;伴生CO2气为有机成因。地质分析认为,渭河盆地固市凹陷具有良好的新生界生物气资源前景,前新生界煤系地层也是渭河盆地重要的潜在烃源岩,表明渭河盆地具有开展进一步油气调查的资源基础。  相似文献   

2.
陕西渭河盆地固市凹陷渭热2井组甲烷气成因及其意义   总被引:1,自引:0,他引:1  
渭河盆地固市凹陷渭热2井组甲烷气的成功点火,再一次引起人们对渭河盆地油气资源前景的关注。渭热2井组及邻区7口井天然气组分、甲烷C同位素等分析指标显示,该区甲烷气具有2种成因类型,浅部气层为新近系张家坡组生物成因气,中深部天然气来自前新生界煤型热解-裂解气;伴生CO2气为有机成因。地质分析认为,渭河盆地固市凹陷具有良好的新生界生物气资源前景,前新生界煤系地层也是渭河盆地重要的潜在烃源岩,表明渭河盆地具有开展进一步油气调查的资源基础。  相似文献   

3.
为了研究固市凹陷深部基底结构特征、为氦等天然气选区评价提供依据,在固市凹陷布置了D1和D2两条大地电磁测深剖面,开展大地电磁测深及综合解释评价工作。本次研究首先对固市凹陷的大地电磁测深剖面的电性特征进行定性分析,再结合二维地震剖面进行约束对其进行定量解释,划分出固市凹陷的主要地层及埋深,确定了新生界张家坡组为氦等天然气资源储集有利层位的深度和厚度。根据本次研究结果显示,大地电磁测深反演结果与地震勘探解释结果相吻合,有效反映了固市凹陷深部地层构造的真实形态,为进一步研究固市凹陷基底结构特征和氦气勘探提供借鉴。  相似文献   

4.
根据天然气组分以及碳同位素和轻烃特征等资料,运用天然气成因理论并结合天然气成因类型判识图版和成藏条件,探讨了潍北凹陷孔店组天然气成因类型及分布规律。结果表明:潍北凹陷天然气CH4体积分数大,重烃体积分数小,非烃组分极少;南部斜坡带的疃4井天然气属生物气;灶户鼻状构造带南部产出的天然气为混有生物气的油型伴生气;灶户鼻状构造带中部地区属典型的油型伴生气;北部洼陷区的东部和南缘产出的天然气具有煤型气,并有油型气混入;以昌1井为代表的北部深洼陷区是煤型气发育的有利地区。总之,潍北凹陷天然气可以划分为生物气、混有生物气的油型伴生气、典型的油型伴生气、混有油型气的煤型气、典型的煤型气等5种成因类型;孔店组天然气类型多样、分布复杂,这些与该区的烃源岩类型、成熟度等因素有关。  相似文献   

5.
冀中坳陷武清凹陷是华北油田公司勘探与研究程度低、研究难度大的地区之一,多年来一直未取得重大进展。以武2井新近系馆陶组获得气流为线索,着重对武清凹陷的岩相古地理环境、有机地化特征、沉积特征、成藏条件、构造特征和资源评价等方面进行了阐述,从而表明武清凹陷浅层生物气具有巨大的勘探潜力。武清凹陷新近系为滨浅湖与河流沼泽相沉积,地层沉积巨厚,广泛发育暗色泥岩,具有浅层生物气形成的基础,有机地化指标良好,盆地模拟计算生物气资源量潜力巨大,天然气主要生成于新近纪,总生气量856×108m3,天然气资源量(150~200)×10.8m3。新近系馆陶组的河道砂体是生物气的良好储集层。新近系沉降速率快,厚度大,埋藏深,有利于生物气的形成和保存。后期构造反转形成的凹中挤压塌陷背斜是生物气聚集的有利场所。  相似文献   

6.
固市凹陷非常规水溶甲烷气成因及来源   总被引:1,自引:0,他引:1  
针对渭河盆地固市凹陷水溶甲烷气的成因类型进行分析研究。对地层水溶甲烷气碳同位素δ13C1及重烃的含量研究发现,不同层位的水溶甲烷气成因类型不同。新近系张家坡组水溶甲烷气主要为有机成因的生物气,来源于本层含碳质较高的灰黑色泥灰岩生物分解,为自生自储式;下部蓝田—灞河组水溶甲烷气以未成熟的煤型热解气(煤型腐殖型)为主,来源于下部地层。对CO2碳同位素的分布范围和含量进行分析得出,δ13CCO2 < -10‰,为典型的壳源型有机成因,证明蓝田—灞河组水溶甲烷气和CO2来源于下部地层的混合型气,结合乙烷碳同位素分析,得出下部地层可能存在有机成因的煤型热解气层系。   相似文献   

7.
根据天然气地球化学基本理论,对柴达木盆地西部(柴西)地区天然气的地球化学特征进行分析。测试和收集该地区18个油气田及含油气构造的83个天然气样品,分析其组分和C同位素数据,结果显示,该区天然气以烃类气体为主,烃类含量介于79.24%~99.81%之间,天然气比重介于0.72~1.36之间,天然气干燥系数(C1/C2+)介于1.04~617.8之间,甲烷C同位素值介于-51.4‰~-24.2‰之间,乙烷C同位素值介于-34.2‰~-17.4‰之间。在此基础上,对该区不同构造带的天然气成因类型进行研究。研究结果表明,柴达木盆地西部地区天然气类型可划分为腐泥型气、腐殖型气、混合气3类,柴西北部天然气主要为腐泥型气和混合气,少量腐殖型气;柴西南部主要为腐泥型气,少量混合气。同时,建立了天然气成因类型的判识指标,对该区的天然气地球化学特征有了较为深入的认识,对今后的天然气勘探具有指导意义。  相似文献   

8.
近年来,由于全球资源量的需求增多,作为勘探程度较低的渭河盆地受到了越来越多学者的关注。而制约渭河盆地油气勘探的主要矛盾是缺乏烃源岩,若盆地存在上古生界烃源岩,则具有重要油气地质意义,可为氦载体气成藏提供物质基础。为了研究渭河盆地及周缘上古生界残留地层分布特征,本文系统收集、整理了渭河盆地及周缘已有地球物理资料,结合地质、地震、钻井、地球化学等研究成果,明确了研究区上古生界残留地层分布,通过对比盆地南北缘上古生界烃源岩特征,探讨渭河盆地内部上古生界天然气勘探潜力。结果表明,渭河盆地内确实存在上古生界地层,主要位于西安凹陷和固市凹陷内,固市凹陷中煤系地层的厚度较西安凹陷大,且厚度较大处靠近南部。烃源岩产生的甲烷气通过盆地内大量的断裂运移到新生界断层封闭的圈闭构造中成藏,新生代地层中发育优质的储盖组合,新近系张家坡组上部分布大范围的湖泛沉积泥岩,构成了良好的区域性盖层,为天然气提供了有利的保存条件。此外,天然气藏的存在可为盆地内氦气成藏提供基础条件。对渭河盆地基底气源岩认识的深化,为鄂尔多斯周缘盆地群油气基础地质调查提供重要的借鉴意义。  相似文献   

9.
孙浩  张敏  李素梅 《现代地质》2013,27(5):1173-1179
由于松辽盆地南部浅层天然气成因研究比较薄弱,通过采集伏龙泉地区泉头组天然气样品,对天然气组分、碳同位素、轻烃组分进行了分析。结果表明该地区天然气有油型气和生物降解气2种成因。第一类天然气甲烷碳同位素值在-35‰左右,甲烷及其同系物碳同位素呈正碳分布;甲基环己烷指数在20%左右、环己烷指数略高于10%,符合油型气的特征。由甲烷碳同位素计算的R0值,以及轻烃中的庚烷值和异庚烷值均在高-过成熟的范围,因此是高成熟的油型气。第二类天然气甲烷碳同位素偏轻,丙烷碳同位素偏重;轻烃色谱图中以环烷烃为主峰,轻烃内组成中支链烷烃和环烷烃含量高,各项轻烃参数(甲基环己烷指数、庚烷值、K1值等)都在较大范围内波动,为生物降解气。这一研究对于今后该区天然气勘探与资源评价及其成藏机理研究具有重要意义。  相似文献   

10.
李钰  符彩云 《地下水》2015,(1):185-187
沉积相的研究对渭河盆地天然气勘探开发具有重要意义。通过构造背景、野外露头、岩性组合、沉积构造等资料的综合研究,分析总结渭河盆地张家坡组和蓝田灞河组沉积相,沉积相类型及沉积特征。结论表明,蓝田灞河组主要以洪积相,河流相,浅湖相为主;张家坡组主要以稳定的湖相沉积为主,经历了浅-深-浅湖的完整发展旋回。  相似文献   

11.
This paper reports the first results of a study of 11 isotope systems (3He/4He, 40Ar/36Ar, 34S/32S, 65Cu/63Cu, 62Ni/60Ni, 87Sr/86Sr, 143Nd/144Nd, 206–208Pb/204Pb, Hf–Nd, U–Pb, and Re–Os) in the rocks and ores of the Cu–Ni–PGE deposits of the Norilsk ore district. Almost all the results were obtained at the Center of Isotopic Research of the Karpinskii All-Russia Research Institute of Geology. The use of a number of independent genetic isotopic signatures and comprehensive isotopic knowledge provided a methodic basis for the interpretation of approximately 5000 isotopic analyses of various elements. The presence of materials from two sources, crust and mantle, was detected in the composition of the rocks and ores. The contribution of the crustal source is especially significant in the paleofluids (gas–liquid microinclusions) of the ore-forming medium. Crustal solutions were probably a transport medium during ore formation. Air argon is dominant in the ores, which indicates a connection between the paleofluids and the atmosphere. This suggests intense groundwater circulation during the crystallization of ore minerals. The age of the rocks and ores of the Norilsk deposits was determined. The stage of orebody formation is restricted to a narrow age interval of 250 ± 10 Ma. An isotopic criterion was proposed for the ore-bearing potential of mafic intrusions in the Norilsk–Taimyr region. It includes several interrelated isotopic ratios of various elements: He, Ar, S, and others.  相似文献   

12.
最新的流行病学研究表明,空气中较高浓度的悬浮细颗粒可能对人类的健康有不利的影响。根据该项研究显示,由于心脏病、慢性呼吸问题和肺功能指标恶化而导致死亡率的升高与细尘粒子有关。这些研究结果已经促使欧盟于1999年4月出台了限制空气中二氧化硫、二氧化氮、氧化氮、铅和颗粒物含量的法案(1999/30/EC),对各项指标包括对可吸入PM10颗粒的浓度提出了新的限制性指标。PM10颗粒是指可以通过预分级器分离采集的气体动力学直径小于10μm的细颗粒。目前研究的兴趣重点逐步偏向PM2.5这些更细微颗粒物,PM2.5这种颗粒物对健康有明显的不利影响。在欧盟指令2008/50/EC中,对PM10和PM2.5都提  相似文献   

13.
Komatiites are mantle-derived ultramafic volcanic rocks. Komatiites have been discovered in several States of India, notably in Karnataka. Studies on the distribution of trace-elements in the komatiites of India are very few. This paper proposes a simple, accurate, precise, rapid, and non-destructive wavelength-dispersive x-ray fluorescence (WDXRF) spectrometric technique for determining Sc, V, Cr, Co, Ni, Cu, Zn, Rb, Sr, Y, Zr, Nb, Ba, Pb, and Th in komatiites, and discusses the accuracy, precision, limits of detection, x-ray spectral-line interferences, inter-element effects, speed, advantages, and limitations of the technique. The accuracy of the technique is excellent (within 3%) for Sc, V, Cr, Co, Ni, Cu, Zn, Rb, Sr, Zr, Nb, Ba, Pb, and Th and very good (within 4%) for Y. The precision is also excellent (within 3%) for Sc, V, Cr, Co, Ni, Cu, Zn, Rb, Sr, Y, Zr, Nb, Ba, Pb, and Th. The limits of detection are: 1 ppm for Sc and V; 2 ppm for Cr, Co, and Ni; 3 ppm for Cu, Zn, Rb, and Sr; 4 ppm for Y and Zr; 6 ppm for Nb; 10 ppm for Ba; 13 ppm for Pb; and 14 ppm for Th. The time taken for determining Sc, V, Cr, Co, Ni, Cu, Zn, Rb, Sr, Y, Zr, Nb, Ba, Pb, and Th in a batch of 24 samples of komatiites, for a replication of four analyses per sample, by one operator, using a manual WDXRF spectrometer, is only 60 hours.  相似文献   

14.
Most sulfide-rich magmatic Ni-Cu-(PGE) deposits form in dynamic magmatic systems by partial melting S-bearing wall rocks with variable degrees of assimilation of miscible silicate and volatile components, and generation of barren to weakly-mineralized immiscible Fe sulfide xenomelts into which Ni-Cu-Co-PGE partition from the magma. Some exceptionally-thick magmatic Cr deposits may form by partial melting oxide-bearing wall rocks with variable degrees of assimilation of the miscible silicate and volatile components, and generation of barren Fe ± Ti oxide xenocrysts into which Cr-Mg-V ± Ti partition from the magma. The products of these processes are variably preserved as skarns, residues, xenoliths, xenocrysts, xenomelts, and xenovolatiles, which play important to critical roles in ore genesis, transport, localization, and/or modification. Incorporation of barren xenoliths/autoliths may induce small amounts of sulfide/chromite to segregate, but incorporation of sulfide xenomelts or oxide xenocrysts with dynamic upgrading of metal tenors (PGE > Cu > Ni > Co and Cr > V > Ti, respectively) is required to make significant ore deposits. Silicate xenomelts are only rarely preserved, but will be variably depleted in chalcophile and ferrous metals. Less dense felsic xenoliths may aid upward sulfide transport by increasing the effective viscosity and decreasing the bulk density of the magma. Denser mafic or metamorphosed xenoliths may also increase the effective viscosity of the magma, but may aid downward sulfide transport by increasing the bulk density of the magma. Sulfide wets olivine, so olivine xenocrysts may act as filter beds to collect advected finely dispersed sulfide droplets, but other silicates and xenoliths may not be wetted by sulfides. Xenovolatiles may retard settling of – or in some cases float – dense sulfide droplets. Reactions of sulfide melts with felsic country rocks may generate Fe-rich skarns that may allow sulfide melts to fractionate to more extreme Cu-Ni-rich compositions. Xenoliths, xenocrysts, xenomelts, and xenovolatiles are more likely to be preserved in cooler basaltic magmas than in hotter komatiitic magmas, and are more likely to be preserved in less dynamic (less turbulent) systems/domain/phases than in more dynamic (more turbulent) systems/domains/phases. Massive to semi-massive Ni-Cu-PGE and Cr mineralization and xenoliths are often localized within footwall embayments, dilations/jogs in dikes, throats of magma conduits, and the horizontal segments of dike-chonolith and dike-sill complexes, which represent fluid dynamic traps for both ascending and descending sulfides/oxides. If skarns, residues, xenoliths, xenocrysts, xenomelts, and/or xenovolatiles are present, they provide important constraints on ore genesis and they are valuable exploration indicators, but they must be included in elemental and isotopic mass balance calculations.  相似文献   

15.
《Applied Geochemistry》2001,16(2):137-159
Five hundred and ninety-eight samples of terrestrial moss (Hylocomium splendens and Pleurozium schreberi) collected from a 188,000 km2 area of the central Barents region (NE Norway, N Finland, NW Russia) were analysed by ICP-AES and ICP-MS. Analytical results for Al, B, Ba, Ca, K, La, Mg, Mn, Na, P, Rb, Si, Sr, Th, U and Y concentrations are reported here. Graphical methods of data analysis, such as geochemical maps, cumulative frequency diagrams, boxplots and scatterplots, are used to interpret the origin of the patterns for these elements. None of the elements reported here are emitted in significant amounts from the smelting industry on the Kola Peninsula. Despite the conventional view that moss chemistry reflects atmospheric element input, the nature of the underlying mineral substrate (regolith or bedrock) is found to have a considerable influence on moss composition for several elements. This influence of the chemistry of the mineral substrate can take place in a variety of ways. (1) It can be completely natural, reflecting the ability of higher plants to take up elements from deep soil horizons and shed them with litterfall onto the surface. (2) It can result from naturally increased soil dust input where vegetation is scarce due to harsh climatic conditions for instance. Alternatively, substrate influence can be enhanced by human activity, such as open-cast mining, creation of ‘technogenic deserts’, or handling, transport and storage of ore and ore products, all of which magnify the natural elemental flux from bedrock to ground vegetation. Seaspray is another natural process affecting moss composition in the area (Mg, Na), and this is most visible in the Norwegian part of the study area. Presence or absence of some plant species, e.g., lichens, seems to influence moss chemistry. This is shown by the low concentrations of B or K in moss on the Finnish and Norwegian side of the (fenced) border with Russia, contrasting with high concentrations on the other side (intensive reindeer husbandry west of the border has selectively depleted the lichen population).  相似文献   

16.
The Kuskokwim River at Bethel, Alaska, drains a major mercury-antimony metallogenic province in its upper reaches and tributaries. Bethel (population 4000) is situated on the Kuskokwim floodplain and also draws its water supply from wells located in river-deposited sediment. A boring through overbank and floodplain sediment has provided material to establish a baseline datum for sediment-hosted heavy metals. Mercury (total), arsenic, antimony, and selenium contents were determined; aluminum was also determined and used as normalizing factor. The contents of the heavy metals were relatively constant with depth and do not reflect any potential enrichment from upstream contaminant sources.  相似文献   

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19.
《Chemical Geology》2007,236(1-2):13-26
We examined the coprecipitation behavior of Ti, Mo, Sn and Sb in Ca–Al–Mg fluorides under two different fluoride forming conditions: at < 70 °C in an ultrasonic bath (denoted as the ultrasonic method) and at 245 °C using a Teflon bomb (denoted as the bomb method). In the ultrasonic method, small amounts of Ti, Mo and Sn coprecipitation were observed with 100% Ca and 100% Mg fluorides. No coprecipitation of Ti, Mo, Sn and Sb in Ca–Al–Mg fluorides occurred when the sample was decomposed by the bomb method except for 100% Ca fluoride. Based on our coprecipitation observations, we have developed a simultaneous determination method for B, Ti, Zr, Nb, Mo, Sn, Sb, Hf and Ta by Q-pole type ICP-MS (ICP-QMS) and sector field type ICP-MS (ICP-SFMS). 9–50 mg of samples with Zr–Mo–Sn–Sb–Hf spikes were decomposed by HF using the bomb method and the ultrasonic method with B spike. The sample was then evaporated and re-dissolved into 0.5 mol l 1 HF, followed by the removal of fluorides by centrifuging. B, Zr, Mo, Sn, Sb and Hf were measured by ID method. Nb and Ta were measured by the ID-internal standardization method, based on Nb/Mo and Ta/Mo ratios using ICP-QMS, for which pseudo-FI was developed and applied. When 100% recovery yields of Zr and Hf are expected, Nb/Zr and Ta/Hf ratios may also be used. Ti was determined by the ID-internal standardization method, based on the Ti/Nb ratio from ICP-SFMS. Only 0.053 ml sample solution was required for measurement of all 9 elements. Dilution factors of ≤ 340 were aspirated without matrix effects. To demonstrate the applicability of our method, 4 carbonaceous chondrites (Ivuna, Orgueil, Cold Bokkeveld and Allende) as well as GSJ and USGS silicate reference materials of basalts, andesites and peridotites were analyzed. Our analytical results are consistent with previous studies, and the mean reproducibility of each element is 1.0–4.6% for basalts and andesites, and 6.7–11% for peridotites except for TiO2.  相似文献   

20.
The Samchampi-Samteran alkaline igneous complex (SAC) is a near circular, plug-like body approximately 12 km2 area and is emplaced into the Precambrian gneissic terrain of the Karbi Anglong district of Assam. The host rocks, which are exposed in immediate vicinity of the intrusion, comprise granite gneiss, migmatite, granodiorite, amphibolite, pegmatite and quartz veins. The SAC is composed of a wide variety of lithologies identified as syenitic fenite, magnetite ± perovskite ± apatite rock, alkali pyroxenite, ijolite-melteigite, carbonatite, nepheline syenite with leucocratic and mesocratic variants, phonolite, volcanic tuff, phosphatic rock and chert breccia. The magnetite ± perovskite ± apatite rock was generated as a cumulus phase owing to the partitioning of Ti, Fe at a shallow level magma chamber (not evolved DI = O1). The highly alkaline hydrous fluid activity indicated by the presence of strongly alkalic minerals in carbonatites and associated alkaline rocks suggests that the composition of original melt was more alkalic than those now found and represent a silica undersaturated ultramafic rock of carbonated olivine-poor nephelinite which splits with falling temperature into two immiscible fractions—one ultimately crystallises as alkali pyroxenite/ijolite and the other as carbonatite. The spatial distribution of varied lithotypes of SAC and their genetic relationships suggests that the silicate and carbonate melts, produced through liquid immiscibility, during ascent generated into an array of lithotypes and also reaction with the country rocks by alkali emanations produced fenitic aureoles (nephelinisation process). Isotopic studies (δ18O and δ13C) on carbonatites of Samchampi have indicated that the δ13C of the source magma is related to contamination from recycled carbon.  相似文献   

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