Study on the Length of Cross-Bay Bridge at Tieshan Port     

YOU Lixin MIAO Difan Engineer  No. Harbour Engineering Investigation  Design Institute of the Ministry of Communications of China  Wuhan  P. R. China 《中国海洋工程》1999,(4)

To determine the optimal length of the cross-bay bridge at the Tieshan Port and the impact ofthe bridge on the hydrological environment,a 2-D numerical model is adopted to calculate the variation oftidal level,tidal current field and tidal discharge caused by different lengths of the bridge.  相似文献   

Constraining the surface properties of Saturn's icy moons, using Cassini/CIRS emissivity spectra     

J.M. Carvano  A. Migliorini  A. Barucci  the CIRS Team 《Icarus》2007,187(2):574-583

We have conducted a search for emissivity features in the thermal infrared spectrum of the icy satellites of Saturn, Phoebe, Iapetus, Enceladus, Tethys, and Hyperion, observed by the Composite Infrared Spectrometer (CIRS) on board the Cassini spacecraft. Despite the heterogeneity of the composition of these bodies depicted by Earth-based and Cassini/VIMS observations, the CIRS spectra of all satellites are undistinguishable from black-body spectra, with no detectable emissivity feature. However, several materials, which have been detected on the surface of the same bodies, present emissivity features in the analyzed spectral range. In particular, water ice presents features with sufficient contrast to be detected by CIRS. Here we study the physical causes of the absence of features by simulating the effects of intimate mixtures using models of directional emissivity for optically thick surfaces for different particle sizes and abundances, and porosities. The simulations include a set of materials detected on the Phoebe's surface, like water ice, hydrated silicates, and organics. We find that featureless spectra can be produced in three scenarios: (1) ice particles with large sizes, (2) mixtures of ices dominated by dark contaminants, and (3) small particles with large porosity. Constraints imposed by the NIR spectra of the satellites favors the latter scenario as the more likely explanation to the absence of emissivity features on the icy satellites of Saturn.  相似文献   

In memory of Vladimir Ivanovich Kononov     

Laboratory of Heat  Mass Transfer  Geological Institute  Russian Academy of Sciences  Scientific Council of the Russian Academy of Sciences on Problems of Geothermy 《Lithology and Mineral Resources》2006,41(4):399-400

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Electrical properties of Titan's surface from Cassini RADAR scatterometer measurements     

Lauren C. Wye  Howard A. Zebker  Richard D. West  Ralph D. Lorenz  the Cassini RADAR Team 《Icarus》2007,188(2):367-385

We report regional-scale low-resolution backscatter images of Titan's surface acquired by the Cassini RADAR scatterometer at a wavelength of 2.18-cm. We find that the average angular dependence of the backscatter from large regions and from specific surface features is consistent with a model composed of a quasi-specular Hagfors term plus a diffuse cosine component. A Gaussian quasi-specular term also fits the data, but less well than the Hagfors term. We derive values for the mean dielectric constant and root-mean-square (rms) slope of the surface from the quasi-specular term, which we ascribe to scattering from the surface interface only. The diffuse term accommodates contributions from volume scattering, multiple scattering, or wavelength-scale near-surface structure. The Hagfors model results imply a surface with regional mean dielectric constants between 1.9 and 3.6 and regional surface roughness that varies between 5.3° and 13.4° in rms-slope. Dielectric constants between 2 and 3 are expected for a surface composed of solid simple hydrocarbons, water ice, or a mixture of both. Smaller dielectric constants, between 1.6 and 1.9, are consistent with liquid hydrocarbons, while larger dielectric constants, near 4.5, may indicate the presence of water-ammonia ice [Lorenz, R.D., 1998. Icarus 136, 344-348] or organic heteropolymers [Thompson, W.R., Squyres, S.W., 1990. Icarus 86, 336-354]. We present backscatter images corrected for angular effects using the model residuals, which show strong features that correspond roughly to those in 0.94-μm ISS images. We model the localized backscatter from specific features to estimate dielectric constant and rms slope when the angular coverage is within the quasi-specular part of the backscatter curve. Only two apparent surface features are scanned with angular coverage sufficient for accurate modeling. Data from the bright albedo feature Quivira suggests a dielectric constant near 2.8 and rms slope near 10.1°. The dark albedo feature Shangri-La is best fit by a Hagfors model with a dielectric constant close to 2.4 and an rms slope near 9.5°. From the modeled backscatter curves, we find the average radar albedo in the same linear (SL) polarization to be near 0.34. We constrain the total-power albedo in order to compare the measurements with available groundbased radar results, which are typically obtained in both senses of circular polarization. We estimate an upper limit of 0.4 on the total-power albedo, a value that is significantly higher than the 0.21 total albedo value measured at 13 cm [Campbell, D., Black, G., Carter, L., Ostro, S., 2003. Science 302, 431-434]. This is consistent with a surface that has more small-scale structure and is thus more reflective at 2-cm than 13-cm. We compare results across overlapping observations and observe that the reduction and analysis are repeatable and consistent. We also confirm the strong correlations between radar and near-infrared images.  相似文献   

Genetic Relationship between Natural Gas Dispersal Zone and Uranium Accumulation in the Northern Ordos Basin, China          下载免费PDF全文

GAN Huajun XIAO Xianming LU Yongchao JIN Yongbin TIAN Hui LIU Dehan 《《地质学报》英文版》2007,81(3):501-509

The Ordos Basin is well-known for the coexistence of oil, natural gas, coal and uranium. However, there has been little research to discuss the genetic relationship between them. In this paper, a case study of the Zaohuohao area in Dongsheng, Inner Mongolia, China, is conducted to investigate the genetic relationship between the natural gas and the uranium accumulation. Fluid inclusion data from the uranium-bearing sandstone samples indicate that the fluid inclusions formed in a gas-water transition zone. Using the homogeneous temperatures of aqueous inclusions coeval with hydrocarbon-bearing inclusions, combined with the buried history and paleo-temperature data, the gas-water transition zone reached the area at about 110 Ma. On the basis of this, the contents of Uranium （U） and Total Organic Carbon （TOC） of the samples were analyzed, and there was no obvious relation between them. With regard to the available data from both publications and this study, it is found that the U mineralization has a spatiotemporal accordance with the gas-water dispersal zone. Thus, it is believed that the natural gas in the gas-water zone is an effective reducer to the U-bearing ground water abundant in oxygen, which is the main factor to U accumulation. This result can be used as the reference to the U mines predicting and prospecting.  相似文献   

塔河地区奥陶系油田水分布与运动学特征研究   总被引：1，自引：0，他引：1       下载免费PDF全文

张金川唐玄  边瑞康云露 王敏王艳芳  杨振恒刘丽芳 《地质学报》2007,81(8):1135-1142

塔河油田是我国最大的陆上整装碳酸盐岩油田,其油田水分布与运动特征反映了油气运移规律。该区奥陶系油田水现今总体矿化度高,南北向存在从低到高再到低的3个矿化带,各带内平面分割性强,纵向层间差异大。塔河油田奥陶系的流体经历了多期次活动,奥陶系储层共捕获了4～5期盐水包裹体,其均一温度范围集中在60～80℃,90～105℃,110～140℃和145～170℃,盐度集中在0.5%～4%、5%～10%、10%～13%、14%～18%、>18%,反映出奥陶系储层曾经历过了4～5期热流体活动,对照埋藏史与油气运移史,高盐度流体活动与油气运移具有良好的匹配关系,油田水化学指标(油田水变质系数、碳酸盐岩平衡系数等)反映出塔河油区现今保存条件良好。井剖面包裹体纵向温度、盐度纵向不规则变化表明流体的活动以侧向运移为主。流体势分析说明运移方向不仅包括塔河东、南面是烃源岩方向,而且具有高流体势的西面也可能是油气来源方向。  相似文献   

Yin-bo QIAN Xian-mei RAO Rui-z     

hong WANG Ying-jian 《大地构造与成矿学》2007,(3)

the multiple phase screen method,could numerically simulate the turbulence effects,thermal blooming and their mutual effects for laser atmospheric propagation. Four types of propagation paths and ten kinds of optical turbulence profiles are also included into the program, which make it possible to simulate the propagating process and the atmospheric effects for laser beam with a circular or rectangular aperture under currently available conditions.Moreover,the beam propagating process can be visualized simultaneously by utilizing open graphics library (OpenGL).With the friendly user interface  相似文献   

Sm-Nd isotopic system in garnet megacrysts from the Udachnaya kimberlite pipe (Yakutia) and petrogenesis of kimberlites     

A. M. Agashev  N. P. Pokhilenko  V. G. Mal’kovets  Academician of the RAS N. V. Sobolev 《Doklady Earth Sciences》2006,407(2):491-494

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The major cyclicity of Mesozoic epicontinental sedimentation and geodynamic events in the adjacent active oceanic region     

P. V. Markevich  Corresponding Member of the RAS A. I. Khanchuk  I. V. Kemkin  V. V. Golozubov  Yu. D. Zakharov 《Doklady Earth Sciences》2006,407(1):184-187

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A Study on the Mesoscale Convective Systems during the Summer Monsoon Onset over the South China Sea in 1998Part I: Analysis of Large-Scale Fields for Occurrence and Development of the Mesoscale Convective Systems     

LIU Yanju  DING Yihui  ZHAO Nan 《Acta Meteorologica Sinica》2005,19(3):275-288

1. Introduction China is located in the East Asian monsoon re- gion. Every year's weather and climate in this region is deeply affected by the monsoon activities. Es- pecially, during flooding season (May to September), the summer monsoon controls large-scale precipitation patterns, the movement of seasonal rain belt and oc- currence of drought/flood disasters. The Asian mon- soon can be divided into two systems (Tao and Chen, 1987). As a major component and its unique location, the South …  相似文献