武乡区块山西组泥页岩孔隙结构及分形特征研究     

曹磊  郭英海 《岩石矿物学杂志》2020,39(3):283-290

沁水盆地东部煤系伴生泥页岩广泛发育,页岩气资源潜力大,开展该区泥页岩孔隙结构特征的研究对页岩含气性评价及实现煤层气、页岩气合探共采具有重要意义。本文以盆地内武乡区块Y井二叠系山西组泥页岩为研究对象,通过XRD、高压压汞和低温液氮吸附等实验手段对泥页岩孔隙结构特征及分形特征进行了研究。结果表明,Y井山西组泥页岩的矿物组成以黏土矿物和石英为主;泥页岩中小于50 nm的孔隙大量发育,结构形态上以狭缝平板型孔隙和"细瓶颈"孔隙为主;泥页岩样品吸附曲线呈倒S型,属于Brunauer分类方案中的Ⅱ型曲线,其脱附曲线属于IUPAC分类方案中的H2型(兼具H1型及H3型),属De Boer分类方案中的B型(兼具E型及C型); Y井山西组泥页岩分形维数接近3,非均质性较强,矿物成分、总孔体积、平均孔径和TOC含量是影响泥页岩分形维数的重要因素。  相似文献   

黔西北地区龙马溪组页岩有机质和脆性矿物的控缝机制     

袁余洋  刘永林  王瑛 《岩石矿物学杂志》2020,39(6):808-818

页岩"甜点"层段中有机质和脆性矿物对裂缝的发育具有极为重要的控制作用，揭示并把握裂缝萌生、发育和演化的机理与规律，对于压裂目标层段的优选以及页岩气增产和稳产具有极为重要的工程实践价值。以黔西北地区龙马溪组页岩为例，通过地化测试、岩石力学实验以及扫描电镜，深入剖析和揭示了"甜点"层段中与有机质和脆性矿物相关的控缝机制，并结合数值模拟实验展现了"甜点"层段中裂缝的形成和演化的完整过程。研究结果表明，有机质和脆性矿物的同步富集为裂缝的发育和演化提供了重要的物质基础，其中裂缝趋向于沿着有机质形成的结构面传播，有机质的孔隙结构对裂缝具有较为明显的诱导机制。在外力作用下，内在积累的能量转化为脆性矿物的变形和变位，脆性矿物含量越高者裂缝发育能力越强，裂缝发育程度越高。数值模拟实验呈现了一种由于有机孔隙和脆性矿物所导致的应力集中从而诱发裂缝萌生和演化的整个过程。该研究成果可为深化认识裂缝的成因机理以及压裂施工过程中相关压裂参数的调整提供一定的借鉴与参考。  相似文献   

Early star formation and the evolution of the stellar initial mass function in galaxies     

Richard B. Larson 《Monthly notices of the Royal Astronomical Society》1998,301(2):569-581

It has frequently been suggested in the literature that the stellar IMF in galaxies was top-heavy at early times. This would be plausible physically if the IMF depended on a mass-scale such as the Jeans mass that was higher at earlier times because of the generally higher temperatures that were present then. In this paper it is suggested, on the basis of current evidence and theory, that the IMF has a universal Salpeter-like form at the upper end, but flattens below a characteristic stellar mass that may vary with time. Much of the evidence that has been attributed to a top-heavy early IMF, including the ubiquitous G-dwarf problem, the high abundance of heavy elements in clusters of galaxies, and the high rate of formation of massive stars in high-redshift galaxies, can be accounted for with such an IMF if the characteristic stellar mass was several times higher during the early stages of galaxy evolution. However, significant variations in the mass-to-light ratios of galaxies and large amounts of dark matter in stellar remnants are not as easily explained in this way, because they require more extreme and less plausible assumptions about the form and variability of the IMF. Metal-free 'population III' stars are predicted to have an IMF that consists exclusively of massive stars, and they could help to account for some of the evidence that has been attributed to a top-heavy early IMF, as well as contributing importantly to the energetics and chemical enrichment of the early Universe.  相似文献   

High-velocity stars from decay of small stellar systems     

L. G. Kiseleva    J. Colin    B. Dauphole  & P. Eggleton 《Monthly notices of the Royal Astronomical Society》1998,301(3):759-766

In this paper we present numerical results on the decay of small stellar systems under different initial conditions (multiplicity 3 ≤  N  ≤ 10, and various mass spectra, initial velocities and initial configurations). The numerical treatment uses the CHAIN1 code (Mikkola &38; Aarseth). Particular attention is paid to the distribution of high-velocity escapers: we define these as stars with velocity above 30 km s⁻¹. These numerical experiments confirm that small N -body systems are dynamically unstable and produce cascades of escapers in the process of their decay. It is shown that the fraction of stars that escape from small dense stellar systems with an escape velocity greater than 30 km s⁻¹ is ∼1 per cent for all systems treated here. This relatively small fraction must be considered in relation to the rate of star formation in the Galaxy in small groups: this could explain some moderately high-velocity stars observed in the Galactic disc and possibly some young stars with relatively high metallicity in the thick disc.  相似文献   

Stellar models for very low-mass main-sequence stars: the role of model atmospheres     

Brocato  Cassisi  & Castellani 《Monthly notices of the Royal Astronomical Society》1998,295(3):711-724

We present very low-mass stellar models as computed using non-grey model atmospheres for selected assumptions about the stellar metallicities. The role of atmospheres is discussed and the models are compared with models based on the Eddington approximation, and with similar models that have appeared in the recent literature. Theoretical predictions concerning both the HR diagram location and the mass–luminosity relation are presented and discussed in terms of expectations in selected photometric bands. Comparison with available observational data concerning both galactic globular clusters and dwarfs in the solar neighbourhood reveals a satisfactory agreement together with the existence of some residual mismatches.  相似文献   

Fine structure of the red giant clump from Hipparcos data, and distance determinations based on its mean magnitude     

Léo Girardi  Martin A. T. Groenewegen  Achim Weiss  & Maurizio Salaris 《Monthly notices of the Royal Astronomical Society》1998,301(1):149-160

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滩间山金矿田成矿作用演化及成因类型     

国家辉 《青海国土经略》1998,(1)

作者对滩间山金矿田成矿作用的演化及其成矿模式进行了概括;同时对其成因类型归属和成矿时代提出了看法。  相似文献   

伊犁石炭纪裂谷的时空演化特征     

金海龙  张成立 《地球科学与环境学报》1998,20(2):48

通过对伊犁盆地石炭纪裂谷火山岩的地层学、岩石学、岩石地球化学等方面的论述,分析了裂谷的形成与演化,探讨了裂谷形成的区域动力学背景。认为裂谷期火山活动具幕式喷发的特点;随着时代的演替,裂谷由初始裂陷的察布查尔－伊什基里克一带扩展到整个伊犁地块;裂谷的形成主要与中天山南北两侧古洋壳的相向俯冲所导致的地幔物质上涌、中上地壳的背向伸展有关。  相似文献   

胶南造山带中高压、超高压变质矿     

王来明  宋明春  刘建文 《山东国土资源》1998,(1)

胶南造山带榴辉岩中的高压、超高压变质矿物主要有绿辉石、镁铝榴石、柯石英、金刚石、金红石等。柯石英、金刚石均呈微晶状包裹于石榴子石、绿辉石中。柯石英多已转化为石英聚晶,并使包裹它的矿物产生放射状胀裂纹;金刚石呈近等轴八面体等,其形成压力达３．５ＧＰａ以上。榴辉岩围岩中的高压、超高压变质矿物主要有辉石类（透辉石、霓石、暗硬玉）、钠钙质钠质角闪石（钠闪石、镁钠闪石）、多硅白云母（３Ｔ型）、钠长石、绿帘石等。高压、超高压变质矿物的广泛出现指示区内存在两期高压变质作用：早期为超高压榴辉岩相变质作用;晚期为高压绿片岩相榴辉岩相变质作用。华北板块与扬子板块的多次碰撞是区内高压、超高压变质作用产生的主要原因。  相似文献   

Socioeconomic Correlates of Increasing Crime Rates in Smaller Communities     

William V. Ackerman 《The Professional geographer》1998,50(3):372-387

This research analyzes changes in crime rates by city size and determines the extent to which these changes can be explained by socioeconomic variables. More particularly it addresses rates of change in mean crime rates for violent and property crime between 1976–1984 and 1985–1994 for all U. S. cities, then compares results to Ohio cities. It provides a detailed analysis of changing crime rates in 111 Ohio cities with populations between 10,000 and 99,999 inhabitants and attempts to account for crime differentials between these cities employing linear regression and factor analysis. Results indicate that crime is significantly related to poverty and its associated conditions and processes.  相似文献