层序成因动力学参数类型及意义

层序地层学为沉积盆地分析的一个重要手段和方法。层序地层学在沉积盆地分析中的参数包括宏观参数和微观参数。宏观参数特指沉积盆地中同一成因类型或成因相关的层序构成的层序组合体的总体特征,主要包括物质组成、宏观轮廓及叠置序列等。微观参数系指单个层序本身的识别标志,分为层序内部标志和层序界面标志。前者包括层序的几何形态、规模级别、内部构型、成因格架和充填序列等;后者包括界面的物理标识、剖面特征、成因属性和级别类型等。不同的层序参数类型揭示不同的成因背景,反映不同的动态过程和成因动力学意义。通过这些参数类型及其成因意义的研究,可分析层序形成与沉积盆地及板块构造的关系,进而研究层序的形成背景和成因动力学,最终为盆地动力学研究提供基础。     

旅游供给的二维组合态势与创新开发模式--我国西部12省(区)案例

以省（区）为单元进行西部旅游资源丰度与区位度组合研究.以2002年和2003年西部12省（区）A级以上景区（点）为样本,计算旅游供给丰度与区位度及其排序.结合聚类与位序分析,发现其呈现出两种类型：低区位、低丰度类型和高区位、高丰度类型.基于二维组合,给出对应的旅游创新开发模式与转化策略.得出如下结论：1）通过对旅游资源丰度和区位的定量分析,可理性地提出准确的开发思路;2）西部旅游资源创新开发必须进行旅游生产力布局与建设.     

Section of Permian deposits and fusulinids in the Halvan Mountains, Yazd province, Central Iran

The Permian section situated northwest of Tabas in the Halvan Mountains is studied and fusulinids occurring in the section are described. The Chili, Sartakht, and Hermez formations distinguished in the section are separated by horizons of bauxitic laterite and belong to the Khan Group formerly ranked as a synonymous formation. Fusulinids occur at two levels in the section. The lower one confined to the Chili Formation yields the so-called Kalaktash fusulinid assemblage of the late Sakmarian age. The second late Asselian assemblage has been discovered in pebbles from conglomerate-breccia in the basal laterite of the Sartakht Formation. A brief characterization of fusulinids is presented and three new species are described. The new Benshiella genus is discriminated from the Rugosofusulinidae family. As Skinner and Wilde (1965, 1966) changed the original diagnosis of the Pseudofusulina genus, we suggest, regarding all species, which have been attributed to this genus but do not satisfy the new diagnosis, as representing the new Nonpseudofusulina genus.     

新疆西准噶尔晚古生代以来构造样式与变形序列研究

断裂构造的发育是不同地质历史、不同应力场条件下地壳应变的叠加。针对某一地域断裂构造的研究,理清其发育序次和不同阶段断裂系统对应的构造应力场,是了解区域大地构造性质演变的重要环节。新疆西准噶尔地区构造运动和岩浆活动非常强烈,是认识中亚构造域性质的重要研究基地,同时也为断裂构造和变形序次研究提供了很好的野外实验室。通过对研究区1500个构造面理产状数据的统计与分析,认为新疆西准噶尔地区主要发育以下几组构造面理：（1）290°走向;（2）10°~20°和80~90°走向;（3）40°~45°和320°~325°走向;（4）60°~70°和340°~350°走向。通过对野外构造现象、断裂之间的交切关系、断裂与相关地层及岩体的切割关系等的综合分析,结合遥感图像解译,确立了走滑断裂是西准噶尔地区晚古生代以来主要的构造样式,并建立了相应的变形序列：（1）大约在二叠纪晚期-三叠纪,由于准噶尔与中天山汇聚末期的区域性水平运动,受到北西-南东向的挤压应力作用,发育最早一期北西西向（290°左右）右旋走滑断裂;（2）侏罗纪-白垩纪,地层产状平缓,没有发现区域性构造变形证据;（3）古近纪,主要受制于太平洋构造域,受到北西-南东向挤压应力作用,发育北北东向（10°~20°）左旋与近东西向（80°~90°）右旋共轭走滑构造;（4）新近纪早期,受印度大陆和欧亚大陆碰撞的远程效应影响,应力场为近南北向,发育北东向（40°~45°）、北西向（320°~325°）走滑构造,新近纪晚期应力场发生了小角度顺时针旋转,构造形迹又转变为北东东向（60°~70°）和北北西向（340°~350°）。     

喀左盆地九佛堂组露头高分辨率层序地层划分

在实测106 km剖面和对喀左盆地九佛堂组沉积特征及演化进行详细研究的基础上,依据相序关系,并结合碳酸钙、油页岩的成因意义,将九佛堂组划分了 1个长期基准面旋回和7个中期基准面旋回。在长期基准面旋回内,上升期的中期基准面旋回发育以上升半旋回为主的不完全对称型中期基准面旋回,上升与下降过渡期的中期基准面旋回,则发育近完全对称的中期基准面旋回,下降期的中期基准面旋回,则发育以下降半旋回为主的不完全对称型中期基准面旋回。经过对中期基准面旋回和短期基准面旋回发育特点和形成原因的详细研究,对代表剖面进行了中期基准面旋回对比。     

苏德尔特构造带贝14块兴安岭群层序地层分析

以层序地层学理论为指导,利用岩心、测井、地震资料相结合的分析手段,建立了苏德尔特构造带贝14块兴安岭群的层序地层等时格架,将兴安岭群划分为3个三级层序和短期中期基准面旋回。分析了个层序的主要构型及其成因,认为盆地由断陷向凹陷转化,沉积速率也随之降低,盆地各层序的厚度由厚变薄。兴安岭群内部层序界面多为沉积间断,不同沉积时期的岩性、物性以及沉积物叠置关系具有明显的韵律性变化。层序发育明显受构造活动的控制,幕式构造活动是构成层序主要构型的成因。     

用测井曲线自动划分层序地层研究

无论在基础地质研究还是在指导沉积矿产资源勘查中 ,层序地层划分都具有重要的作用。利用测井资料进行人工层序地层划分是一项重要工作 ,但效率较低。根据层序地层划分的原则 ,采用频谱分析和砂泥岩比值方法设计了层序地层划分的自动算法 ,在济阳坳陷部分区块进行了应用 ,取得了较好的效果 ,为层序地层划分提供了有效的工具。     

皇城山银矿床地球化学特征及预测评价

皇城山银矿床是近年勘查评价出的一处中型低温银矿床.矿床赋存于中生代早白垩世火山岩、次火山岩内,矿体产于北东向花岗斑岩脉中,且严格受火山构造控制.矿区普查阶段比较系统地开展了万分之一岩石测量和原生晕找盲矿专题研究.通过对皇城山银矿地球化学特征研究,建立找矿评价标志,进而对矿带未知地段进行分析对比,做出深部远景评价,取得较好的地质找矿效果.     

X‐shooting Herbig Ae/Be stars: Accretion probed by near‐infrared He I emission

The Herbig Ae/Be stars are intermediate mass pre‐main sequence stars that bridge the gap between the low mass T Tauri stars and the Massive Young Stellar Objects. In this mass range, the acting star forming mechanism switches from magnetically controlled accretion to an as yet unknown mechanism, but which is likely to be direct disk accretion onto the star. We observed a large sample of Herbig Ae/Be stars with X‐shooter to address this issue from a multi‐wavelength perspective. It is the largest such study to date, not only because of the number of objects involved, but also because of the large wavelength coverage from the blue to the near‐infrared. This allows many accretion diagnostics to be studied simultaneously. By correlating the various properties with mass, temperature and age, we aim to determine where and whether the magnetically controlled mass accretion mechanism halts and the proposed direct disk accretion takes over. Here, we will give an overview of the background, present some observations and discuss our initial results. We will introduce a new accretion diagnostic for the research of Herbig Ae/Be stars, the HeI 1.083 μm line (© 2011 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

The Permian Kas Formation of SE Turkey—palynological correlation with strata from Saudi Arabia and Oman

The Kas Formation in SE Turkey was deposited as part of the Permian sequence on the northern margin of the Arabian Plate. Its stratigraphic relationship to time‐equivalent strata of the Arabian Plate was mentioned briefly in previous studies, but has not been elaborated and illustrated in detail. This biostratigraphic review of existing palaeontological data has improved the accuracy of age interpretation for the Kas Formation, and the relationship of its excellent palynological record to the international Permian chronostratigraphic units. As a result, this study has identified a number of key palynological species from the Kas Formation, which occur as well as in the ‘Basal Khuff Clastics’ of Saudi Arabia and in the ‘Khuff transition section’ of Oman. All these units have approximately the same age: Wordian to early Capitanian, based on ‘age control’ provided by Foraminifera. This study also demonstrates that, by using key palynological taxa, correlation of strata would be possible across the entire Arabian Plate in this narrow time range. Hence, the ‘Oman and Saudi Arabia Palynological Zone 6’ (OSPZ6) is applicable throughout the Arabian Plate area, including the northern regions of SE Turkey and Iraq. Copyright © 2011 John Wiley & Sons, Ltd.