Magmatic History of Somma-Vesuvius on the Basis of New Geochemical and Isotopic Data from a Deep Borehole (Camaldoli della Torre)

A continuous-coring borehole recently drilled at Camaldoli dellaTorre on the southern slopes of Somma–Vesuvius providesconstraints on the volcanic and magmatic history of the Vesuvianvolcanic area since c. 126 ka BP. The cored sequence includesvolcanic units, defined on stratigraphical, sedimentological,petrological and geochemical grounds, emitted from both localand distal vents. Some of these units are of known age, suchas one Phlegraean pre-Campanian Ignimbrite, Campanian Ignimbrite(39 ka), Neapolitan Yellow Tuff (14· 9 ka) and VesuvianPlinian deposits, which helps to constrain the relative ageof the other units. The main rock types encountered are shoshonite,phonotephrite, latite, trachyte and phonolite. The sequenceincludes, from the base upwards: a thick succession of pyroclasticunits emplaced between 126 and 39 ka, most of them attributedto eruptions that occurred in the Phlegraean area; the CampanianIgnimbrite; the products of a local tuff cone formed between39 ka and the deposition of the products of the earliest activityof the Mt. Somma volcano; the products of the Somma–Vesuviusvolcano, which include from the base upwards a thick sequenceof lavas, pyroclastic rocks and the products of a local spattercone dated between 3· 7 ka and AD 79. The data obtainedfrom the study of the borehole show that, before the CampanianIgnimbrite eruption, low-energy explosive volcanism took placein the Vesuvian area, whereas mostly high-energy explosive eruptionscharacterized the Campi Flegrei activity. In the Vesuvian area,Campanian Ignimbrite deposition was followed by the eruptionof a local tuff cone and a long repose time, which predatedthe formation of the Mt. Somma edifice. Since 18· 3 ka(Pomici di Base eruption) the activity of Somma–Vesuviusbecame mostly explosive with rare lava effusions. The shallowestcored deposits belong to the Camaldoli della Torre cone, formedbetween the Pomici di Avellino and Pomici di Pompei eruptions(3· 7 ka–AD 79). New geochemical and Sr–Nd–Pb–B-isotopicdata on samples from the drilled core, together with those availablefrom the literature, allow us to further distinguish the volcanicrocks as a function of both their provenance (i.e. Phlegraeanor Vesuvian areas) and age, and to identify different magmaticprocesses acting through time in the Vesuvian mantle source(s)and during magma ascent towards the surface. Isotopically distinctmagmas, rising from a mantle source variably contaminated byslab-derived components, stagnated at mid-crustal depths (8–10km below sea level) where magmas differentiated and were probablycontaminated. Contamination occurred either with Hercynian continentalcrust, mostly during the oldest stages of Vesuvian activity(from 39 to 16 ka), or with Mesozoic limestone, mostly duringrecent Vesuvian activity. Energy constrained assimilation andfractional crystallization (EC-AFC) modelling results show thatcontamination with Hercynian crust probably occurred duringdifferentiation from shoshonite to latite. Contamination withlimestone, which is not well constrained with the availabledata, might have occurred only during the transition from shoshoniteto tephrite. From the ‘deep’ reservoir, magmas rosetowards a series of shallow reservoirs, in which they differentiatedfurther, mixed, and fed volcanic activity. KEY WORDS: Somma–Vesuvius; crustal contamination; source heterogeneity; radiogenic and stable isotopes; magmatic system     

Sedimentary Environments of Cambrian–Ordovician Source Rocks and Ultra-deep Petroleum Accumulation in the Tarim Basin

The Tarim Basin is the only petroliferous basin enriched with marine oil and gas in China. It is presently also the deepest basin for petroleum exploration and development in the world. There are two main sets of marine Source Rocks (SRs) in the Tarim Basin, namely the high over-mature Cambrian–Lower Ordovician (∈–O1) and the moderately mature Middle–Upper Ordovician (O2–3). The characteristic biomarkers of SRs and oils indicate that the main origin of the marine petroleum is a mixed source of ∈–O1 and O2–3 SRs. With increasing burial, the hydrocarbon contribution of the ∈–O1 SRs gradually increases. Accompanied by the superposition of multi-stage hydrocarbon-generation of the SRs and various secondary alteration processes, the emergence and abnormal enrichment of terpenoids, thiophene and trimethylaryl isoprenoid in deep reservoirs indicate a complex genesis of various deep oils and gases. Through the analysis of the biofacies and sedimentary environments of the ∈–O1 and O2–3 SRs, it is shown that the lower Paleozoic high-quality SRs in the Tarim Basin were mainly deposited in a passive continental margin and the gentle slope of the platform, deep-water shelf and slope facies, which has exhibited a good response to the local tectonic-sedimentary environment. The slope of the paleo-uplift is the mutual area for the development of carbonate reservoirs and the deposition of marine SRs, which would be favorable for the accumulation of petroleum. Due to the characteristics of low ground temperature, the latest rapid and deep burial does not cause massive oil-cracking in the paleo-uplift and slope area. Therefore, it is speculated that the marine reservoirs in the slope of the Tabei Uplift are likely to be a favorable area for deep petroleum exploration, while the oil-cracking gas would be a potential reserve around the west margin of the Manjiaer Depression. Hydrocarbons were generated from various unit SRs, mainly migrating along the lateral unconformities or reservoirs and the vertical faults. They eventually brought up three major types of exploration fields: middle and lower Cambrian salt-related assemblages, dolomite inner reservoirs and Middle and Lower Ordovician oil-bearing karst, which would become the most favorable target of marine ultra-deep exploration in the Tarim Basin.     

滇东北松梁铅锌矿床成矿物质来源：来自S、Pb、Zn同位素的证据

川滇黔铅锌多金属成矿域内,碳酸盐岩容矿的热液铅锌矿床多达400个。松梁铅锌矿床地处滇东北与川东南的交接处,位于川滇黔铅锌多金属成矿域的核心部位;铅锌矿体赋存于震旦系灯影组白云岩内,矿体产出明显受断裂控制;矿石矿物组成简单,主要由闪锌矿、方铅矿和黄铁矿组成。文章重点研究了松梁铅锌矿床硫化物的S、Pb、Zn同位素组成,进而探讨了其成矿物质来源及矿床成因。研究表明,松梁铅锌矿床的硫化物δ³⁴S_CDT值在+4.6‰~+13.7‰之间,平均值为+10.5‰,显示硫来源于赋矿围岩,为震旦系灯影组硫酸盐经TSR的产物;硫化物的Pb同位素比值为²⁰⁶Pb/²⁰⁴Pb=18.158~18.513、²⁰⁷Pb/²⁰⁴Pb=15.633~15.895、²⁰⁸Pb/²⁰⁴Pb=38.096~38.786,反映成矿物质为壳源铅,源自震旦系灯影组白云岩与结晶基底的混合;闪锌矿的δ⁶⁶Zn为-0.126‰~+0.082‰,揭示成矿物质可能源自震旦系灯影组碳酸盐岩和结晶基底的混合。松梁铅锌矿床为后生碳酸盐岩容矿型铅锌矿床。     

多源遥感数据在新疆卡拉麦里地区岩矿识别中的应用

遥感技术广泛应用于地质基础调查、矿产资源勘探、环境评估和地质灾害调查等方面。它已从多光谱发展到高光谱阶段,Landsat- 8是目前最具有代表性和最常用的多光谱数据,ASTER具有高的分辨率和多波段特征,资源一号02D(ZY1- 02D)卫星是我国2019年发射的高光谱业务卫星。为了更好地了解多源遥感数据在岩矿识别中的作用,在新疆东天山卡拉麦里地区进行了相关研究。结果表明：Landsat- 8 OLI的PCA变换结果清晰识别了研究区不同的岩性和地层;使用Landsat- 8 OLI、ASTER和ZY1- 02D高光谱数据,分别采取不同的图像端元提取方法,在进行光谱分析的基础上,利用光谱角填图（SAM）即可得到研究区的主要矿物分类图件。通过野外验证,应用GIS技术进行集成和分析,修正相关图件后,便得到了精准的矿物分类综合图。研究表明：多源遥感数据的集成在岩矿识别方面效果良好、前景巨大。     

基于抗转模型的颗粒材料宏−细观关系研究

接触模型的宏?细观参数标定是成功使用离散元方法的关键。在离散元的接触模型中线性接触模型与抗转线性接触模型均可用于模拟砂性土的力学行为,其中抗转线性接触模型在模拟密砂的剪胀性方面具备优势。采用抗转线性接触模型对室内密实砂土三轴试验进行了离散元模拟,验证了抗转线性接触模型的可靠性;进而系统分析了颗粒间摩擦系数、刚度比和抗转动系数等细观参数与砂土峰值内摩擦角、残余内摩擦角、峰值剪胀角等宏观参数的相关关系并进行了验证;揭示了偏应力作用下,细观参数对密实砂土试样内部剪切带宽度与倾角变化的影响规律,提出了考虑剪胀角的剪切带倾角经验公式。通过研究建立了抗转线性接触模型宏?细观参数的量化关系并给出了标定参数的具体流程图,提出了快速标定宏观参数的方法并应用实例进行了验证,为采用抗转线性接触模型精准模拟密实砂土的力学特性提供依据。     

青藏高原腹地各拉丹冬南北坡多年冻土考察初步结果

青藏高原唐古拉山南北两侧在地形地貌、地理和气候特征上存在显著差异,多年冻土的发育状况和特征也明显不同。受第二次青藏高原综合科学考察研究等项目资助,多年冻土对亚洲水塔的影响专题考察分队分别于2019年和2020年的10—11月对唐古拉山各拉丹冬南侧的色林错上游扎加藏布源区（简称“湖源区”）和北侧的长江上游沱沱河源区（简称“江源区”）进行了多年冻土野外考察。利用钻探、坑探、地球物理勘探等方法对多年冻土的分布边界、多年冻土剖面的地层、地下冰等特征进行了描述和取样,同步构建了多年冻土温度和活动层水热观测网络,为多年冻土对亚洲水塔影响的机理分析、数值模拟以及情景预估提供数据保障。对野外调查资料的初步分析认为,各拉丹冬南北两坡地层沉积类型和地下冰赋存状态存在明显差异,北坡多年冻土的热稳定性、地下冰含量、冰缘地貌类型多样性均高于南坡,但由于受到构造地热、河流融区等多种因素的影响,北坡的冻土分布形式更为复杂。江源区100 m钻孔剖面揭示了连续分布的、厚度大于50 m的地下冰;在该区域发现了多年生冻胀丘分布群,并利用钻探和地球物理勘探方法对该区域规模最大、结构最完整的冰核型冻胀丘进行了较为系统的勘察剖析。两次野外调查工作共采集钻孔岩心、表层土壤、冰水等各类样本近1.2万件,为后期区域冻土理化指标分析,冻土环境化学、古气候环境研究的开展奠定基础。     

银额盆地哈日凹陷油气成藏条件及成藏模式

近年来,银额盆地哈日凹陷的油气勘探呈现出良好的态势,但对于哈日凹陷油气成藏条件相关研究甚少,已不能满足目前油气勘探开发的需求。本研究基于钻录井、地球物理、分析化验等资料,系统分析哈日凹陷油气成藏的烃源岩、储层、圈闭等条件,总结油气成藏条件配置关系,以期为哈日凹陷的后续油气勘探及地质研究提供依据。哈日凹陷主要发育三套烃源岩,其中银根组烃源岩有机质丰度极高,成熟度较低,有机质类型为Ⅰ-Ⅱ1型;巴二段烃源岩有机质丰度较高,成熟-高成熟,有机质类型为Ⅱ1-Ⅱ2型;巴一段烃源岩有机质丰度中等,成熟-高成熟,有机质类型为Ⅱ1-Ⅱ2型。储层类型为砂（砾）岩常规储层、碳酸质泥岩非常规储层和火山岩储层,且均属于特低孔超低渗储层,其中砂、砾岩储层和灰质泥岩储层物性最好,白云岩储层和火成岩储层次之,目前主力油藏主要集中在砂、砾岩储层和灰质泥岩储层这两种类型中。哈日凹陷主要发育两套岩性圈闭,即巴一段砂岩岩性圈闭和巴二段泥岩岩性圈闭,形成了源内（准）连续成藏模式和近源不连续成藏模式。     

源外斜坡区有利于油气运聚的断砂配置分布区预测方法

为了研究含油气盆地源外斜坡区油气分布规律,在源外斜坡区断砂配置运聚机制及有利分布区研究的基础上,通过砂体连通分布区和砂体所在地层顶面砂体输导油气汇聚区,确定油气成藏期砂体输导油气分布区;通过断裂填充物泥质含量与断裂侧向封闭所需的最小填充物泥质含量的相对大小,确定油气成藏期河道砂体上倾方向断裂侧向封闭部位,二者叠合建立了一套源外斜坡区有利于油气运聚的断砂配置分布区预测方法,并将其应用于渤海湾盆地歧口凹陷有利于油气运聚的扣村断裂与沙一下亚段砂体配置分布区的预测中。结果表明：有利于油气运聚的扣村断裂与沙一下亚段砂体配置分布区主要分布在其东部,有利于西北歧南次凹沙三段源岩生成油气在扣村断裂附近沙一下亚段内聚集成藏,与目前扣村断裂附近沙一下亚段已发现油气主要分布在其东部相吻合,表明该方法用于预测源外斜坡区有利于油气运聚的断砂配置分布区是可行的。     

基于三维流-固耦合模型的油井出砂细观机制研究

油井出砂机制的研究是提高油藏产能和石油开采成本减小的关键课题,而常规的宏观力学理论和方法不能全面反映油藏开采过程中油井出砂的发生和发展。鉴于砂岩储层的物理性质和射孔试验特征,从岩土力学的角度建立基于柱坐标系的三维颗粒流数值模型,与理论分析成果进行比较,以说明该细观数值模型可行性,有效地模拟出砂过程中的渗流及流-固耦合效应。在该基础上,综合考虑流体压力梯度力和拖曳力,基于PFC3D模型模拟流体不同运动时的砂岩性态。数值分析得到的模型宏观应力图形说明流体运动对砂岩力学特性的影响不可忽略,且在相同条件下,流量越大,砂岩的塑性区越大,形成砂岩破坏出砂的几率也越大。同时,不同工况的砂岩黏结分布和颗粒转动图形表明,相同条件下流量越大,颗粒间平行黏结破坏越多,颗粒转动越大,失去黏结约束的颗粒也越多,出砂量就越大,可见两种细观特征图形与宏观应力图形变化规律一致,该模型可用于油井出砂机制的研究,可为出砂量预测及出砂控制提供新的研究思路。     

内蒙古突泉盆地ZK-WJT钻井下侏罗统红旗组 生烃潜力

对突泉盆地西南缘ZK-WJT井红旗组烃源岩的发育特征和有机质丰度、类型及成熟度的研究表明,下侏罗统红旗组暗色泥岩发育,厚度达113.0m.有机碳的含量分布在0.56％～6.24％之间,平均值为1.90％.应用Pr/n-C17与Ph/n-C18的相关关系及C27、C28、C29甾烷(ααα-20R)三者的相对含量,判断其有机质类型为Ⅱ1型.镜质组反射率R.主要分布于1.26％～1.73％之间,平均值为1.37％;岩石热解参数Tmax主要为489.0～517.0℃,平均值为507.6℃,红旗组烃源岩属于成熟—高成熟演化阶段.综合评价认为,突泉盆地下侏罗统红旗组具备较好的生油气潜力.