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1.
Yu. G. Shkuratov K. Muinonen E. Bowell K. Lumme J. I. Peltoniemi M. A. Kreslavsky D. G. Stankevich V. P. Tishkovetz N. V. Opanasenko L. Y. Melkumova 《Earth, Moon, and Planets》1994,65(3):201-246
About a dozen physical mechanisms and models aspire to explain the negative polarization of light scattered by atmosphereless celestial bodies. This is too large a number for the reliable interpretation of observational data. Through a comparative analysis of the models, our main goal is to answer the question: Does any one model have an advantage over the others? Our analysis is based on new laboratory polarimetric and photometric data as well as on theoretical results. We show that the widely used models due to Hopfield and Wolff cannot realistically explain the phase-angle dependence of the degree of polarization observed at small phase angles. The so-called interference or coherent backscattering mechanism is the most promising model. Models based on that mechanism use well-defined physical parameters to explain both negative polarization and the opposition effect. They are supported by laboratory experiments, particularly those showing enhancement of negative polarization with decreasing particle size down to the wavelength of light. According to the interference mechanism, pronounced negative branches of polarization, like those of C-class asteroids, may indicate a high degree of optical inhomogeneity of light-scattering surfaces at small scales. The mechanism also seems appropriate for treating the negative polarization and opposition effects of cometary dust comae, planetary rings, and the zodiacal light. 相似文献
2.
浊积砂体沉积微相及储层非均质性研究——以东营胜坨油田T74地区古近系沙河街组三段中亚段浊积砂体为例 总被引:1,自引:0,他引:1
利用岩心观察、测井相分析、测井资料处理与评价、图像分析等方法,系统研究了胜坨油田T74地区古近系沙河街组三段中亚段浊积砂体的沉积微相及储层非均质性.研究表明,T74地区沙河街组三段中亚段储层由三期浊积砂体叠加形成,可划分为中心微相和边缘微相两种沉积微相带;各期浊积砂体储层非均质性较强,层内非均质性以韵律性不明显、渗透率差异大为主要特征,层间及平面非均质性主要受沉积微相控制,中心微相储层的物性要好于边缘微相;不同沉积相带储层微观孔隙结构存在差异,中心微相主要发育中孔中喉和细孔中喉型孔隙结构,边缘微相主要发育细孔细喉以及微孔型孔隙结构. 相似文献
3.
The scope of the present paper is to provide analytic solutions to the problem of the attitude evolution of a symmetric gyrostat about a fixed point in a central Newtonian force field when the potential function isV
(2).We assume that the center of mass and the gyrostatic moment are on the axis of symmetry and that the initial conditions are the following: (t
0)=0, (t
0)=0, (t
0)=(t
0)=0, 1(t
0)=0, 2(t
0)=0 and 3(t
0)=
3
0
.The problem is integrated when the third component of the total angular momentum is different from zero (B
1 0). There now appear equilibrium solutions that did not exist in the caseB
1=0, which can be determined in function of the value ofl
3
r
(the third component of the gyrostatic momentum).The possible types of solutions (elliptic, trigonometric, stationary) depend upon the nature of the roots of the functiong(u). The solutions for Euler angles are given in terms of functions of the timet. If we cancel the third component of the gyrostatic momentum (l
3
r
=0), the obtained solutions are valid for rigid bodies. 相似文献
4.
C1相干算法是计算每道的横测线和相邻纵测线的互相关,依据相干值来判断地层和岩性的横向不均匀性。根据互相关原理,提出了相干体算法中二维和三维C1算法的内容及其具体实现。通过对实际三维地震资料的处理,结合已知地质资料,证明C1相干技术在三维地震资料的断层解释方面有着明显的效果。 相似文献
5.
一种基于InSAR相干系数的SAR阴影提取方法 总被引:1,自引:0,他引:1
给出了一种新的阴影提取方法,根据阴影区域在InSAR相干系数图上的特性,利用Sigma滤波和最优阈值分割算法实现阴影的自动提取。实验结果表明,本方法是一种高效的阴影提取方法。 相似文献
6.
7.
8.
ABSTRACT A process‐based facies model for asymmetric wave‐influenced deltas predicts significant river‐borne muds with potentially lower quality reservoir facies in prodelta and downdrift areas, and better quality sand in updrift areas. Many ancient barrier‐lagoon systems and ‘offshore bars’ may be better reinterpreted as components of large‐scale asymmetric wave‐influenced deltaic systems. The proposed model is based on a re‐evaluation of several modern examples. An asymmetry index A is defined as the ratio between the net longshore transport rate at the mouth (in m3 year?1) and river discharge (in 106 m3 month?1). Symmetry is favoured in deltas with an index below ≈ 200 (e.g. Tiber, lobes of the Godavari delta, Rosetta lobe of the Nile, Ebro), whereas deltas with a higher index are asymmetric (e.g. Danube – Sf. Gheorghe lobe, Brazos, Damietta lobe of the Nile). Periodic deflection of the river mouth for significant distances in the downdrift direction occurs in extreme cases of littoral drift dominance (e.g. Mahanadi), resulting in a series of randomly distributed, quasi‐parallel series of sand spits and channel fills. Asymmetric deltas show variable proportions of river‐, wave‐ and tide‐dominated facies both among and within their lobes. Bayhead deltas, lagoons and barrier islands form naturally in prograding asymmetric deltas and are not necessarily associated with transgressive systems. This complexity underlines the necessity of interpreting ancient depositional systems in a larger palaeogeographic context. 相似文献
9.
南黄海潮成辐射砂脊群的面积约为20000km2,以160° 的角度从弓京港向海展开。它与以弓京港为顶点的辐聚辐散潮流场相伴而生。60余个钻孔揭示,毗邻海区辐射砂脊体系的江苏沿岸平原上存在一个面积约3000 km2潮成砂区,其顶点位于东台,同样呈扇形以130°的角度向东展开。在潮成砂区内潮成砂质沉积单元位于冰后期海侵型砂坝-湖沉积层之上,二者之间具明显的冲刷面。砂坝-湖沉积层位于晚更新世基底硬粘土层之上,二者之间有较长的沉积间断。潮成砂沉积层上覆潮坪沉积层,二者呈渐变关系。以潮成砂层底部的侵蚀面为界,其下为海侵序列,其上为海退序列。古潮流的研究揭示,潮成砂区内同样存在辐聚辐散的古潮流场,其顶点位于东台附近。由此推断,沿海平原的潮成砂区内也是辐射状潮成砂脊体系,它形成于全新世海退时期。由于长江和黄河三角洲的前展,以东台为顶点的潮成砂脊体系逐渐暴露成陆。陆上和海域潮成辐射砂脊群形成于相同的潮汐动力环境,但处在不同的发育阶段,前者形成于全新世中期,后者发育于全新世晚期。矿物分析揭示,陆上和海区的潮成辐射砂脊体系主要由长江和黄河沉积物组成,其中长江沉积物由南向北运移,且时间较早;黄河沉积物由北向南运移,时间较迟,这种泥沙的运移趋势一直延续至今。随着海平面上升趋于减缓,长江三角洲增长,江苏海岸线向外推进,苏北潮成砂区逐渐出露成陆。1128年黄河由苏北入海,大量的黄河沉积物的加入,加快了本区海岸线的推进速度。潮成辐射砂脊体系与辐聚辐散的潮流场相伴而生,全新世最大海侵以来,辐聚辐散的潮流场的位置曾经历三次变化,第一次以长江古河口湾为顶点,第二次位于现今陆上潮成砂区,第三次位于以弓京港为顶点的现代海域,代表了潮成辐射砂脊体系发育的三个阶段。只是长江古河口湾的潮成辐射砂脊体系由于河流的巨大改造作用,可能未很好保存,至今未发现典型的辐射砂脊体系。 相似文献
10.
为了加深对黄金带复杂断块油田进一步开发,针对该区断层复杂、储层变化大、油水关系复杂等特征,笔者综合运用岩心、分析化验及录井、测井资料,对其沉积特征、储层岩性、物性和非均质性进行详细研究。以JASON软件为平台,对含油砂体进行了追踪和预测,并在有利区提出井位部署,为该区的进一步开发提供了地质依据。 相似文献