新疆尼勒克县吉仁台沟口遗址石器功能分析:来自植物微体遗存的证据     

王清  马志坤  陈秋荷  马永超  阮秋荣  王永强  韩建业  杨晓燕 《第四纪研究》2020,(2):450-461

新疆地处欧亚大陆中心,自然环境复杂,生业经济形式多样,东西方文化交流频繁,是了解欧亚大陆古代人类活动和文化发展的重要区域.从新石器时代至青铜时代在该区域出土了丰富的石制品,但对其功能的研究较少,尤其是一些中国内地不常见,而与中亚、欧亚草原类型相似的石器.本文对新疆伊犁地区青铜时代吉仁台沟口遗址(82.77°E,43.84°N;3600~3000 cal.a B.P.)出土的具有安德罗诺沃文化特征的长条形石磨盘、石杵和饼形石器的表层残留物进行了淀粉粒和植硅体分析,为这些石器的功能研究提供了直接证据.分析结果显示,石器表面的淀粉粒来自禾本科小麦族(the tribe Triticeae)和某些块根块茎类植物,而石器表面发现的775粒植硅体中,粟类作物稃片植硅体占9%,其他类型的植硅体以早熟禾亚科(Pooideae)型和棒型为主,另在石杵上发现栝楼属(Trichosanthes)植物果皮植硅体及植物组织.结合遗址中大植物遗存证据,研究结果表明:石磨盘曾用于研磨麦类作物种子和某些块根块茎类植物,石杵亦用于麦类作物研磨,但也对粟类作物进行脱壳以及加工栝楼属植物果实.用于分析的饼形石器有两种类型,第一类为打制饼形石器,残留物中的植物遗存显示可能与石磨盘组合用于加工植物的块根块茎;第二类为磨制饼形石器,其表面发现极少量粟类稃片植硅体,推测其可能用于粟类作物脱粒.研究结果为新疆伊犁地区考古遗址出土安德罗诺沃文化石器的功能、农作物加工过程,以及古代社会生计模式的认识提供了依据;石器残留物中块根块茎类淀粉粒以及农作物植硅体的发现,是对已有大植物遗存分析结果的进一步补充.  相似文献   

塔里木盆地志留系沥青砂岩有效厚度的确定方法     

姜振学  庞雄奇  王显东  张俊  李宏义 《地质学报》2006,80(3):418-423

塔里木盆地志留系具有分布广泛的沥青砂岩,沥青砂岩段厚度在各个地区具有不均匀性,从几米到一百多米不等。岩心观察发现沥青砂岩段内并不全含有沥青,岩心剖面上呈现“黑白砂相间”的现象,“黑砂”的部分为含沥青层段,“白砂”的部分为不含沥青层段。弄清“白砂”中曾经是否有油气进入,对志留系沥青砂岩中沥青含量、古油藏油气储量的计算及志留系剩余油气资源量的评价具有重要的意义。本文通过对志留系沥青砂岩段的“黑砂”与“白砂”分别取样,采用物性测定、显微镜下岩性观察、含油包裹体颗粒指数(GOI)数据观测及定量颗粒荧光(QGF)指数测定等多种方法和技术手段对沥青砂岩段的“黑砂”与“白砂”进行对比研究。结果表明,沥青砂岩段的“白砂”没有油气进入或进入的油气量很少,在确定志留系沥青砂岩有效厚度时应剔除“白砂”层的厚度。  相似文献   

基于二维连续小波变换的颗粒物数字粒径方法研究     

郭立恒  刘海江 《海洋工程》2018,36(5):38-48

对于海岸工程的研究而言,测定泥沙、砾石、卵石等颗粒物的中值粒径具有重要的研究意义。近年来,许多学者逐渐将统计学方法应用于分析泥沙等颗粒物的粒径大小及其级配分布,小波变换是该研究领域时新的统计计算数学方法之一。由于一维连续小波变换(1D-CWT)在估算颗粒数值粒径方面存在一定的局限性,本研究基于二维连续小波变换(2D-CWT),提出了新的颗粒物粒径统计学分析方法,用于估算筛分良好的颗粒物中值粒径。以玻璃珠、卵石块和砾石三类不同性质的颗粒物构建数字粒径实验分析样本,对新方法进行了测试和验证。研究表明基于2D-CWT的数字粒径分析方法能够快速、便捷地估算出筛分良好的颗粒物的中值粒径,且计算结果准确、稳定。相较于基于1D-CWT的数字粒径分析方法,2D-CWT方法在颗粒物数字粒径分析方面有着更高的计算成功率和更广的适用性。  相似文献   

Quartz cementation in Late Cretaceous mudstones,northern North Sea: Changes in rock properties due to dissolution of smectite and precipitation of micro-quartz crystals     

Brit Thyberg  Jens JahrenTurid Winje  Knut BjørlykkeJan Inge Faleide  Øyvind Marcussen 《Marine and Petroleum Geology》2010

Late Cretaceous mudstones from two wells located in the northern North Sea and the Norwegian Sea have been examined with respect to quartz cement. Two different types of quartz cement (Type 1 and Type 2) have been identified using SEM/EDS/CL-analysis of drill-bit cuttings at depths 2370–2670 m (80–85 °C). Type 1 appears as relatively large aggregates (30–100 μm) of depth/temperature related crypto- or microcrystalline to macrocrystalline irregular quartz cement formed by local re-crystallization of biogenic silica. The CL-responses of Type 1 quartz cement give a clear indication of an authigenic origin. Type 2 quartz cement represents relatively high amounts of extremely fine-grained micro-sized (1–3 μm) crystals embedded as discrete, short chains or small clusters/nests within the illitized clay matrix. The CL-responses of micro-quartz crystals indicate an authigenic origin. The micro-quartz is most probably sourced from silica released during the smectite to illite dissolution–precipitation reaction. The petrographic evidence indicates that most of the silica released by the smectite to illite reaction has not been exported out of the mudstones. The silica released produce a subtle inter-connected micro-quartz network interlocked with aggregates of micro-quartz and authigenic clay crystals. This micro-quartz cementation process causes a significant and sharp change in the mudstone stiffness at the onset of the chemical compaction regime. This is indicated by an abrupt increase in well log velocity (Vp) and change in seismic facies close to 2500 m (80/85 °C).  相似文献   

Clay mineral diagenesis and quartz cementation in mudstones: The effects of smectite to illite reaction on rock properties   总被引：1，自引：0，他引：1  

Christer Peltonen  Øyvind MarcussenKnut Bjørlykke  Jens Jahren 《Marine and Petroleum Geology》2009

The Late Cretaceous to Early Tertiary sequence of the Vøring and Møre Basins from the Norwegian Sea has been examined with respect to mineralogy based on 319 cutting samples from five wells. A clear relationship between mineralogy and well log data is demonstrated. A significant change with respect to velocity, porosity and density occurs within the depth interval corresponding to 80–90 °C. At shallow depths/temperatures (<2.0 km/70 °C), compaction is mainly mechanical and the physical properties are similar to what has been measured by experimental compaction of mudstones. At greater depths, however, the log derived velocities and densities are higher than those produced by experimental compaction indicating significant chemical compaction. XRD analyses show a progressive alteration of smectite to illite (S–I) within this depth/temperature interval which results in the release of significant amounts of silica into solution. Detrital silt and fine-grained quartz showed no secondary quartz overgrowths. These grains are isolated within a clay matrix and surrounded by clay minerals, thus limiting the available surface area and pore space for quartz overgrowths. Chemical analyses (XRF) indicate that silica is conserved within this depth interval, and the amount released from S–I alteration was locally precipitated. Field emission gun-scanning electron microscopy (FEG-SEM) and cathode luminescence (CL) identified authigenic micro-crystalline quartz cement within the clay matrix at temperatures above ∼85 °C. This is accompanied by an increase in velocity and density indicating that the S–I reaction and the precipitation of authigenic quartz caused a significant change in the rock stiffness.  相似文献   

Beta dose heterogeneity in sediment samples measured using a Timepix pixelated detector and its implications for optical dating of individual mineral grains     

《Quaternary Geochronology》2022

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The SPICE project: Calibrated cosmogenic 26Al production rates and cross-calibrated 26Al /10Be, 26Al/14C,and 26Al/21Ne ratios in quartz from the SP basalt flow,AZ, USA     

《Quaternary Geochronology》2022

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Carbon altotropic composition of interstellar grains     

N. Maron 《Astronomische Nachrichten》1989,310(4):315-317

Extinktionskurven für Kern-Mantel-Teilchen und für Vielkernteilchen, die allotrope Kohlenstoffmodifikationen enthalten, werden mit Extinktionsbeobachtungen der Sterne R CrB und R Y Sgr im fernen UV sowie mit der interstellaren Extinktion verglichen. Wir zeigen, daß dieses Teilchenmodell mit der beobachteten Extinktion im fernen UV verträglich ist, finden jedoch, daß nur Teilchen, in denen amorpher Kohlenstoff von Graphit ist, die interstellare Extinktionskurve und die der R-CrB-Sterne gut wiedergeben.  相似文献