Gravitational imaging of cold dark matter substructures     

L. V. E. Koopmans 《Monthly notices of the Royal Astronomical Society》2005,363(4):1136-1144

  相似文献   

A Method for Determining Sedimentary Micro-Facies Belts Automatically     

Linfu Xue  Qitai Mei  Quan Sun 《世界地质(英文版)》2003,6(1)

It is important to understand the distribution of sedimentary facies, especially the distribution of sand body that is the key for oil production and exploration. The secondary oil recovery requires analyzing a great deal of data accumulated within decades of oil field development. At many cases sedimentary micro-facies maps need to be reconstructed and redrawn frequently, which is time-consuming and heavy. This paper presents an integrated approach for determining the distribution of sedimentary micro-facies, tracing the micro-facies boundary, and drawing the map of sedimentary micro-facies belts automatically by computer technique. The approach is based on the division and correlation of strata of multiple wells as well as analysis of sedimentary facies. The approach includes transform, gridding, interpolation, superposing, searching boundary and drawing the map of sedimentary facies belts, and employs the spatial interpolation method and "worm" interpolation method to determine the distribution of sedimentary micro-facies including sand ribbon and/or sand blanket. The computer software developed on the basis of the above principle provides a tool for quick visualization and understanding the distribution of sedimentary micro-facies and reservoir. Satisfied results have been achieveed by applying the technique to the Putaohua Oil Field in Songliao Basin, China.  相似文献   

On the dipole straylight contamination in spinning space missions dedicated to cosmic microwave background anisotropy     

C. Burigana  A. Gruppuso  F. Finelli 《Monthly notices of the Royal Astronomical Society》2006,371(4):1570-1586

  相似文献   

Models of the formation of the solar nebula     

Patrick Cassen  Audrey Summers 《Icarus》1983,53(1):26-40

Models of the collapse of a protostellar cloud and the formation of the solar nebula reveal that the size of the nebula produced will be the larger of $\text{R}{}_{\mathrm{<mtext>CF</mtext>}}\text{≡ J}{}^2\text{/k}{}^2\text{GM}{}^3\text{and}\text{R}{}_{\mathrm{<mtext>V</mtext>}}\text{≡ (GMv/2c}{}_{\mathrm{<mtext>c</mtext>}}{}^3\text{)}\text{1}\text{2}$ (where J, M, and c_s are the total angular momentum, total mass, and sound speed of the protosetellar material; G is the gravitational constant; k is a number of order unity; and v is the effective viscosity in the nebula). From this result it can be deduced that low-mass nebulas are produced if P ≡ (R_V/R_CF)² ? 1; “massive” nebulas result if P ? 1. Gravitational instabilities are expected to be important for the evolution of P ? 1 nebulas. The value of J distinguishes most current models of the solar nebula, since P ∝ J^?4. Analytic expressions for the surface density, nebular mass flux, and photospheric temperature distributions during the formation stage are presented for some simple models that illustrate the general properties of growing protostellar disks. It does not yet seem possible to rule out either P ? 1 or P < 1 for the solar nebula, but observed or possible heterogeneities in composition and angular-momentum orientation favor P < 1 models.  相似文献   

Analysis on the interplanetary causes of the great magnetic storms in solar maximum (2000-2001)     

X.H. Xue  Yuming Wang  P.Z. Ye  S. Wang  M. Xiong 《Planetary and Space Science》2005,53(4):443-457

In this paper, we analyze the interplanetary causes of eight great geomagnetic storms during the solar maximum (2000-2001). The result shows that the interplanetary causes were the intense southward magnetic field and the notable characteristic among the causal mechanism is compression. Six of eight great geomagnetic storms were associated with the compression of southward magnetic field, which can be classified into (1) the compression between ICMEs (2) the compression between ICMEs and interplanetary medium. It suggests that the compressed magnetic field would be more geoeffective. At the same time, we also find that half of all great storms were related to successive halo CMEs, most of which originated from the same active region. The interactions between successive halo CMEs usually can lead to greater geoeffectiveness by enhancing their southward field B_s interval either in the sheath region of the ejecta or within magnetic clouds (MCs). The types of them included: the compression between the fast speed transient flow and the slow speed background flow, the multiple MCs, besides shock compression. Further, the linear fit of the D_st versus gives the weights of and Δt as α=2.51 and β=0.75, respectively. This may suggest that the compression mechanism, with associated intense B_s, rather than duration, is the main factor in causing a great geomagnetic storm.  相似文献   

A field evaluation of enhanced reductive dechlorination of chlorinated solvents in groundwater,New York Metropolitan Area     

Eric?Rodriguez  Kevin?A.?McGuinness  Duke?U.?OphoriEmail author 《Environmental Geology》2004,45(5):623-632

An initial assessment of an old manufacturing site with groundwater impacted by trichloroethene (TCE) contamination in the metropolitan New York area showed that the TCE was being removed naturally by reductive dechlorination. However, complete dechlorination was not expected at the site because the process was progressing too slowly under transitional to aerobic conditions at a degradation constant of –0.0013 and a TCE half life of 533 days. A pilot test was conducted at the site in which a carbohydrate substrate (molasses) was injected into the groundwater to create an In-Situ Reactive Zone (IRZ). Post-pilot test groundwater sampling and analysis indicated that an IRZ was created successfully as the total organic carbon (TOC) content and conductivity increased significantly while oxidation-reduction (REDOX) potential and dissolved oxygen (DO) decreased. The created IRZ caused enhanced reductive dechlorination of TCE at the site, found to proceed with a degradation constant of –0.0158 and a TCE half life of 44 days.  相似文献   

一种基于网络拓扑关系的地图匹配算法   总被引：3，自引：0，他引：3  

陈波  王茂林  王宏  杨天克 《测绘科学技术学报》2006,23(5):331-334

地图匹配是车辆导航定位系统中提高定位精度的一种方法,其精度受定位数据、地图数据质量及坐标系转换关系的影响.在分析现有算法的基础上,提出了一种基于网络拓扑关系的地图匹配算法.该算法只需将GPS定位数据和GIS 数据相结合,即可用算法的形式解决地图匹配中一些常见的问题.实验证明:该算法是一种精度高、效率好、实用性强的地图匹配算法,具有较好的实用价值.  相似文献   

国外海相油气田勘探实例之三 美国得克萨斯州法尔韦油田     

张跃平 《海相油气地质》2006,11(1):52-62

美国法尔韦油田位于东得克萨斯盆地中心附近。油田发现于1960年,同年投入生产。原始地质储量为4亿桶,至2003年累计产油2.17亿桶。原油具挥发性,接近饱和。主要储层为下白垩统James组礁石灰岩,主要为骨架粒状灰岩/泥粒灰岩和富含双壳类粒泥状灰岩,各岩相的平均孔隙度一般在7%～11%,但平均渗透率在各岩相中不均,最高达(37～44)×10-3"m2。介绍了该油田的勘探史,描述了盆地构造演化史、含油气系统、地层沉积相和储层特征。  相似文献   

玉林市“6·21”大暴雨成因分析     

陈明璐  张洁婷 《广西气象》2010,(4):34-36,48

利用常规的天气图、物理量场及数值预报等资料,对2010年6月21日玉林市出现的大暴雨天气进行分析,结果表明：（1）高空波动、中低层切变线、西南暖湿气流和地面弱冷空气是影响此次强降水过程的主要天气系统;（2）对于单站预报,在掌握大气环流形势背景的同时,综合分析各物理量场尤其是本站的重要物理量各层垂直分布,对预报有很好的指示意义。  相似文献   

高原地区雷暴过程地面电场变化特征分析     

邹事钢  郝俊平  刘佳  张向东  李丹  刘晋联  陈志峰 《山西气象》2010,(2):33-36

高原地区是我国雷暴天气多发区之一。通过对大气电场仪所测得雷电过程地面电场变化特征的分析有助于了解这一地区的雷暴特征,对认识该地区雷暴过程特征有一定的参考价值。对雷暴过程初期的地面电场波形变化的曲线拟合,总结出了共同的特征,为地面电场资料在雷电预警预报中的应用提供了参考价值。对雷暴过程地面电场资料的特征分析以及预报方面的研究都是很有现实意义的。  相似文献