鄂尔多斯盆地樊学油区长8砂岩裂缝平面展布及控制因素

裂缝发育程度及其平面展布是影响低孔特低渗储层有效、高效注水开发的关键。鄂尔多斯盆地樊学油区长8油藏及周边油藏投产油井存在砂岩裂缝发育区含水上升快、裂缝侧向油井水驱开发效率低等问题。本文基于岩心、声电成像测井资料标定常规测井资料,选取特征参数构建裂缝识别综合指数,实现樊学油区长8储层中砂岩裂缝的识别。依据识别结果绘制砂岩裂缝平面展布图,进而结合区域构造应力场及沉积特征分析裂缝发育的控制因素及其对生产开发的影响。研究表明,基底断裂中生代以来的重新活动控制了樊学油区裂缝的形成与展布,裂缝优势展布方位为北北西向和北东东向,砂岩裂缝的发育程度受区域构造应力场、砂体厚度以及岩层组合等因素影响。裂缝发育区油井具有初产高、产量递减快的特点,因此,在实际生产开发中,需要选择合适的注采井网,尽量采用大井距、小排距的方式提高驱油效率。上述认识为油藏开发部署提供一定的参考。     

Applicability of Landsat 8 data for characterizing glacier facies and supraglacial debris

The present work evaluates the applicability of operational land imager (OLI) and thermal infrared sensor (TIRS) on-board Landsat 8 satellite. We demonstrate an algorithm for automated mapping of glacier facies and supraglacial debris using data collected in blue, near infrared (NIR), short wave infrared (SWIR) and thermal infrared (TIR) bands. The reflectance properties in visible and NIR regions of OLI for various glacier facies are in contrast with those in SWIR region. Based on the premise that different surface types (snow, ice and debris) of a glacier should show distinct thermal regimes, the ‘at-satellite brightness temperature’ obtained using TIRS was used as a base layer for developing the algorithm. This base layer was enhanced and modified using contrasting reflectance properties of OLI bands. In addition to facies and debris cover characterization, another interesting outcome of this algorithm was extraction of crevasses on the glacier surface which were distinctly visible in output and classified images. The validity of this algorithm was checked using field data along a transect of the glacier acquired during the satellite pass over the study area. With slight scene-dependent threshold adjustments, this work can be replicated for mapping glacier facies and supraglacial debris in any alpine valley glacier.     

Improved coastal wetland mapping using very-high 2-meter spatial resolution imagery

Accurate wetland maps are a fundamental requirement for land use management and for wetland restoration planning. Several wetland map products are available today; most of them based on remote sensing images, but their different data sources and mapping methods lead to substantially different estimations of wetland location and extent. We used two very high-resolution (2 m) WorldView-2 satellite images and one (30 m) Landsat 8 Operational Land Imager (OLI) image to assess wetland coverage in two coastal areas of Tampa Bay (Florida): Fort De Soto State Park and Weedon Island Preserve. An initial unsupervised classification derived from WorldView-2 was more accurate at identifying wetlands based on ground truth data collected in the field than the classification derived from Landsat 8 OLI (82% vs. 46% accuracy). The WorldView-2 data was then used to define the parameters of a simple and efficient decision tree with four nodes for a more exacting classification. The criteria for the decision tree were derived by extracting radiance spectra at 1500 separate pixels from the WorldView-2 data within field-validated regions. Results for both study areas showed high accuracy in both wetland (82% at Fort De Soto State Park, and 94% at Weedon Island Preserve) and non-wetland vegetation classes (90% and 83%, respectively). Historical, published land-use maps overestimate wetland surface cover by factors of 2–10 in the study areas. The proposed methods improve speed and efficiency of wetland map production, allow semi-annual monitoring through repeat satellite passes, and improve the accuracy and precision with which wetlands are identified.     

Elemental abundance analyses with DAO spectrograms: XXX. The middle B through early A stars ξ2 Ceti (B9 III), 21 Aquilae (B8 II‐III), ι Aquilae (B5 III), and ι Delphini (A2V)

This series of high quality elemental abundance analyses of mostly main‐sequence band normal and peculiar B, A, and F stars defines their properties and provides data for the comparison with the analyses of somewhat similar stars and with theoretical predictions. Most use high dispersion and high S/N (≥ 200) spectrograms obtained with CCD detectors at the long camera of the Coudé spectrograph of the 1.22‐m Dominion Astrophysical Observatory telescope. Here we reanalyze 21 Aql with better quality spectra and increase the number of stars consistently analyzed in the spectral range B5 to A2 by analyzing three new stars for this series. In the early A stars the normal and non‐mCP stars have abundances with overlapping ranges. But more stars are needed especially in the B5 to B9 range. ξ² Cet on average has a solar composition with a few abundances outside the solar range while both 21 Aql and ι Aql have abundances marginally less than solar. The abundances of ι Del are greater than solar with a few elements such as Ca being less than solar. It is an Am star (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

CSAMT法在深部找矿中的应用

CSAMT法是建立MT和AMT的基础上发展起来的一种人工源频率域测深方法,具有勘探深度适中、分辨率高和抗干扰能力强的优点,在金属矿勘探中是一种行之有效的方法。笔者先分析了目的矿区（二连铜矿区）的基本地理条件、地质和地球物理特征,得出该铜矿区深部原生铜矿具有＂低阻高极化特征＂的结论,为CSAMT法攻深找盲提供了前提准备条件;而后又介绍了CSAMT的原理和工作方法,并利用加拿大凤凰公司生产的新一代网络化多功能电法仪V8进行野外数据采集,通过对该矿区数据资料的处理和异常分析,推断解释出异常区域,结果表明,该方法成功解释了矿体深部富集区的位置、埋深和范围,并通过钻孔验证,为二连铜矿的二次开发提供了依据,成功地体现出了CSAMT法在攻深找盲中的应用的有效性。     

Practical aspects of demand and capacity evaluation of RC members in the context of EC8‐3

The structural safety assessment procedures proposed in Part 3 of Eurocode 8 (EC8‐3) for the case of reinforced concrete structures are addressed. The practical evaluation of the member chord rotation demand according to EC8‐3 is examined in detail along with several alternative formulations. The need for these formulations is demonstrated by presenting example situations where the EC8‐3 proposal is difficult to apply. The effectiveness of the proposed approaches is assessed through an example application and recommendations for their practical use are defined. Given the importance of the shear span in this context, a sensitivity analysis of the EC8‐3 capacity models with respect to this parameter is carried out and discussed in a later section. This analysis aims to assess the validity of the simplifications proposed by a previous research study for the quantification of the EC8‐3 capacity values. Copyright © 2009 John Wiley & Sons, Ltd.     

A displacement‐based seismic design procedure for RC buildings and comparison with EC8

A procedure for displacement‐based seismic design (DBD) of reinforced concrete buildings is described and applied to a 4‐storey test structure. The essential elements of the design procedure are: (a) proportioning of members for gravity loads; (b) estimation of peak inelastic member deformation demands in the so‐designed structure due to the design (‘life‐safety’) earthquake; (c) revision of reinforcement and final detailing of members to meet these inelastic deformation demands; (d) capacity design of members and joints in shear. Additional but non‐essential steps between (a) and (b) are: (i) proportioning of members for the ULS against lateral loads, such as wind or a serviceability (‘immediate occupancy’) earthquake; and (ii) capacity design of columns in flexure at joints. Inelastic deformation demands in step (b) are estimated from an elastic analysis using secant‐to‐yield member stiffnesses. Empirical expressions for the deformation capacity of RC elements are used for the final proportioning of elements to meet the inelastic deformation demands. The procedure is applied to one side of a 4‐storey test structure that includes a coupled wall and a two‐bay frame. The other side is designed and detailed according to Eurocode 8. Major differences result in the reinforcement of the two sides, with significant savings on the DBD‐side. Pre‐test calculations show no major difference in the seismic performance of the two sides of the test structure. Copyright © 2001 John Wiley & Sons, Ltd.     

强震前中期地震活动的变化及TIP预测研究

用改进的Ｍ８算法研究了１９７９年以来我国华北西南及邻近地区共１６次强震前的ＴＩＰ，即震发生概率增长时间。结果表明，１４次强震发生在补判定为概率增长时间的ＴＩＰ内。ＴＩＰ警戒约占研究部时空域的３７％，获得了较好的强震中期预测内符效果。表明该方法可作为强震中期预测的手段之一。     

白云石的微化反应与有序度

试验证实白云石的微化反应特征明显受有序度的影响，白云石粉末在稀盐酸中的起泡程度随有序度的降低而加剧，在茜素红溶液中的染色程度和速度随有序度的降低而增强。低有序度白云石或完全无序的原白云石，其微化反应与方解石极为相似，反之，高有序度白云石与菱镁矿相似。另外还讨论白云石微化反应的机理。     

Performance of the stereoscopic system of the HEGRA imaging air erenkov telescopes: Monte Carlo simulations and observations

Based on the Monte Carlo simulations we have studied the performance of the HEGRA system of imaging air erenkov telescopes (IACTs) in its present configuration of 4 IACTs as well as in its future final configuration of 5 IACTs. Here we present the results on the basic characteristics of the IACT system which are used in the standard data analysis procedure, i.e., the collection areas, the detection rates, the angular resolution, the energy resolution, and the γ/hadron-separation efficiency. By comparing several key Monte Carlo predictions with experimental results it is possible to check the accuracy of the simulations. The Monte Carlo results concerning hadron-nuclear showers are tested with the recorded cosmic ray events and the results concerning photon-induced showers are tested with a large data sample of γ-rays observed from BL Lac object Mkn 501 during its high flaring activity in 1997. Summarizing the simulations and current observations we give the basic recommendations of using the instrument and the major values of its sensitivity.