塔里木盆地塔中地区奥陶系古岩溶包裹体特征及古环境意义     

张庆玉  李景瑞  梁彬  淡永  曹建文 《中国岩溶》2020,39(6):894-899

碳酸盐岩古岩溶型储层是油气勘探开发的重点领域,具有极强的非均质性,是世界级难题。古岩溶发育期次的确定一直都是古岩溶储层地质建模的技术难题。现有判别古岩溶发育期次的方法多以地表裸露古岩溶充填物特征为依据。在塔里木盆地塔中地区地质构造复杂,具有多期次古岩溶作用的叠加改造。本次利用古岩溶充填方解石流体包裹体均一温度法,研究塔中地区奥陶系碳酸盐岩古岩溶作用期次与古环境条件,揭示了4期古岩溶作用环境:加里东期古岩溶作用、海西晚期古岩溶作用、印支-燕山期古岩溶作用、喜马拉雅期古岩溶作用。该研究成果对后期岩溶储层预测具有重要意义。   相似文献   

蜀南Z工区茅口组顶岩溶古地貌、古水系特征与刻画     

聂国权  淡永  李景瑞  徐亮 《中国岩溶》2020,39(6):911-917

蜀南地区茅口组灰岩岩溶储层较为发育,是蜀南地区重要的产层之一。但是该套储层非均质性强、缝洞充填程度高,储层预测具有较大困难。恢复岩溶古地貌、刻画古水系,可以摸清岩溶储层的发育分布规律,对蜀南地区茅口组油气勘探具有重要的指导意义。本文利用印模-趋势面法,以茅口组顶至长兴组顶的沉积厚度为标识,恢复了蜀南Z工区的岩溶古地貌,根据微地貌组合形态,划分了4类三级地貌单元,并结合岩溶水文地质学理论在Z工区刻画出南北向地表水系。分析认为不同的地貌位置,水动力条件具有较大差异;河流两侧位于径流区,水动力条件最强,溶蚀孔缝最发育,是下一步储层勘探方向。   相似文献   

黏声介质平面波有限差分叠前深度偏移及在莺歌海盆地的应用          下载免费PDF全文

李添才  谢玉洪  李列  王华忠  王新领  但志伟  胡江涛 《地球物理学报》2014,57(5):1612-1622

莺琼盆地诸探区中存在底劈现象,深层气源产生的气体沿底劈产生的裂隙通道向上漫溢.漫溢过程中,一是充填在遇到的砂体中形成气藏;二是弥漫在上溢通道中,使得通道中的纵波速度发生变化,进而纵波波阻抗差异变小,反射变弱.另外,通道中气体的存在,会加强地层的吸收衰减,使得地震波振幅变弱、高频成分损失导致同相轴分辨率降低.利用OBC数据进行多波地震勘探和利用黏声介质的叠前深度偏移都是改善模糊区成像质量的重要方法技术.为此,本文提出用黏声介质平面波有限差分法叠前深度偏移成像方法改善气体充填区域的成像质量.黏声介质成像目的是补偿地震波的吸收衰减;平面波偏移成像目的是适应海上单炮数量巨大,提高波动方程叠前深度偏移成像的效率;有限差分法叠前偏移的目的是适应该区浅层气分布局域性极强、Q值的空间变化大的情况.在莺歌海某探区的实际数据上的黏声介质平面波有限差分叠前深度偏移试验证明,本方法是改善模糊区成像质量的较为有效的途径.  相似文献   

The dayside magnetospheric boundary layer at Mercury     

Brian J. Anderson  James A. Slavin  Haje Korth  Scott A. Boardsen  Thomas H. Zurbuchen  Jim M. Raines  George Gloeckler  Ralph L. McNutt Jr.  Sean C. Solomon 《Planetary and Space Science》2011,59(15):2037-2050

Magnetic field and plasma data from the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft on the outbound portions of the first (M1) and second (M2) flybys of Mercury reveal a region of depressed magnetic field magnitude and enhanced proton fluxes adjacent to but within the magnetopause, which we denote as a dayside boundary layer. The layer was present during both encounters despite the contrasting dayside magnetic reconnection, which was minimal during M1 and strong during M2. The overall width of the layer is estimated to be between 1000 and 1400 km, spanning most of the distance from the dayside planetary surface to the magnetopause in the mid-morning. During both flybys the magnetic pressure decrease was ∼1.6 nPa, and the width of the inner edge was comparable to proton gyro-kinetic scales. The maximum variance in the magnetic field across the inner edge was aligned with the magnetic field vector, and the magnetic field direction did not change markedly, indicating that the change in field intensity was consistent with an outward plasma-pressure gradient perpendicular to the magnetic field. Proton pressures in the layer inferred from reduced distribution observations were 0.4 nPa during M1 and 1.0 nPa during M2, indicating either that the proton pressure estimates are low or that heavy ions contribute substantially to the boundary-layer plasma pressure. If the layer is formed by protons drifting westward from the cusp, there should be a strong morning–afternoon asymmetry that is independent of the interplanetary magnetic field (IMF) direction. Conversely, if heavy ions play a major role, the layer should be strong in the morning (afternoon) for northward (southward) IMF. Future MESSENGER observations from orbit about Mercury should distinguish between these two possibilities.  相似文献   

Measurement of the radius of Mercury by radio occultation during the MESSENGER flybys     

Mark E. Perry  Daniel S. Kahan  Olivier S. Barnouin  Carolyn M. Ernst  Sean C. Solomon  Maria T. Zuber  David E. Smith  Roger J. Phillips  Dipak K. Srinivasan  Jürgen Oberst  Sami W. Asmar 《Planetary and Space Science》2011,59(15):1925-1931

The MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft completed three flybys of Mercury in 2008–2009. During the first and third of those flybys, MESSENGER passed behind the planet from the perspective of Earth, occulting the radio-frequency (RF) transmissions. The occultation start and end times, recovered with 0.1 s accuracy or better by fitting edge-diffraction patterns to the RF power history, are used to estimate Mercury's radius at the tangent point of the RF path. To relate the measured radius to the planet shape, we evaluate local topography using images to identify the high-elevation feature that defines the RF path or using altimeter data to quantify surface roughness. Radius measurements are accurate to 150 m, and uncertainty in the average radius of the surrounding terrain, after adjustments are made from the local high at the tangent point of the RF path, is 350 m. The results are consistent with Mercury's equatorial shape as inferred from observations by the Mercury Laser Altimeter and ground-based radar. The three independent estimates of radius from occultation events collectively yield a mean radius for Mercury of 2439.2±0.5 km.  相似文献   

Seismic and Petrophysical Relationships from UK Continental Shelf Rocks at Elevated Pressures     

Solomon Assefa  Clive Mc Cann  Jeremy Sothcott 《Marine Georesources & Geotechnology》2013,31(2):119-140

Abstract

There are few published seismic (P- and S-waves) properties for seafloor bedrocks. At low pressures (1 to 10 MPa), velocities and attenuations are determined mainly by open microcracks. At higher pressures, the microcracks close, and the velocities and attenuations depend primarily on the matrix porosity. We have investigated both the relationships between the acoustic, petrophysical, and geological properties of the rocks at 40 MPa pressure and the effect of microcracks on the acoustic properties at 10 MPa pressure. In this paper we discuss the former; the latter will be discussed separately.

P- and S-wave velocity and attenuation measurements were carried out on a suite of seabed sedimentary and igneous rocks at effective pressures from 10 to 40 MPa at ultrasonic frequencies. The porosities and permeabilities of the rocks ranged from 0% to 32% and 0 to 110 mDarcy, respectively. Characterization of the rocks revealed that most of the sandstones have a substantial clay content (kaolinite, illite, and chlorite) and fractures. Most of the igneous rocks are chloritized.

The seismic properties of the rocks are markedly lower than those of similar continental rocks because of the microporosity formed by the alteration of feldspars, micas, and mafic minerals to clays (e.g., chloritization of pyroxenes) and the corresponding reduction of the elastic moduli. The results of this study suggest that the values of velocities and quality factors used for ocean acoustic propagation models are lower than normally assumed.  相似文献   

塔里木盆地塔北露头区的古岩溶发育模式     

张庆玉  梁彬  曹建文  淡永  郝彦珍  李景瑞 《海洋地质前沿》2013,(12):32-36

目前塔里木盆地海相碳酸盐岩的油气勘探已进入高峰期,为弥补钻井岩心资料不足,进一步认识井下岩溶发育规律及发育模式特征,开展塔北露头区奥陶系风化壳古岩溶缝洞系统发育特征及发育模式研究。研究表明,岩溶发育主要受控于岩性因素和不整合面,主要发育层位为一间房组地层;主要岩溶作用期为吐木休克组／一间房组沉积间断岩溶期。为井下岩溶缝洞系统的认识及岩溶地质模型的建立提供了重要理论依据。  相似文献   

全球变暖背景下新疆地区近45 a来最大冻土深度变化及其突变分析     

符传博  丹利  吴涧  魏荣庆 《冰川冻土》2013,35(6):1410-1418

利用覆盖新疆大部分地区资料完整的93个站点资料,对1961-2005年新疆地区最大冻土深度进行了分析. 结果表明：新疆地区月最大冻土深度有明显的季节变化,低海拔区域(海拔<1 800 m)最大值出现在1月份,而高海拔区域(海拔≥1 800 m)的最大值出现在2月份,比低海拔区域要滞后. 新疆地区最大冻土深度的地理分布特征表现为北疆深于南疆,山区深于平原,且与气温的分布有很好的一致性. 全年和冬、春季最大冻土深度与气温场的空间相关系数分别为-0.795、-0.736和-0.848. 年际变化表明,近45 a来的最大冻土深度出现了较为明显的下降. 高海拔区域与低海拔区域年最大冻土深度的倾向率分别为-15.65 cm·(10a)^-1和-9.48 cm·(10a)^-1,且与气温的相关系数分别为-0.51和-0.69,均通过了0.001的信度检验. 同时发现,高海拔区域冬季下降多,而低海拔区域春季下降多. 新疆地区年最大冻土深度在近45 a有明显的突变现象,高海拔区域和低海拔区域突变发生年份分别为1996/1997年度和1978/1979年度,说明新疆地区高海拔区域的年最大冻土深度对气温变化的响应比低海拔区域要滞后. 突变年后高海拔区域与低海拔区域年最大冻土深度比突变年前的平均值分别降低了61.12 cm和26.67 cm.  相似文献   

Rotational sensors—a comparison of different sensor types     

Felix Bernauer  Joachim Wassermann  Heiner Igel 《Journal of Seismology》2012,16(4):595-602

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南京长江新济洲群湿地保护与恢复规划设计   总被引：1，自引：0，他引：1  

吴后建  但新球  舒勇 《湿地科学与管理》2008,4(4):40-42

以南京长江新济洲群湿地为例,分析了在长江中下游开展洲滩湿地生态恢复的重要意义和必要性,在分析了南京长江新济洲群湿地退化现状及其驱动因素的基础上,对其保护和恢复规划设计进行了探讨,希望为长江中下游洲滩湿地的保护和生态恢复提供思路和借鉴。  相似文献