Stratigraphic,sedimentological and palaeoenvironmental constraints on the rise of the Urgonian platform in the western Swiss Jura     

ALEXIS GODET  KARL B. FÖLLMI  STÉPHANE BODIN  ERIC De KAENEL  VIRGINIE MATERA  THIERRY ADATTE 《Sedimentology》2010,57(4):1088-1125

Urgonian‐type carbonates are a characteristic feature of many late Early Cretaceous shallow‐marine, tropical and subtropical environments. The presence of typical photozoan carbonate‐producing communities including corals and rudists indicates the prevalence of warm, transparent and presumably oligotrophic conditions in a period otherwise characterized by the high density of globally occurring anoxic episodes. Of particular interest, therefore, is the exploration of relationships between Urgonian platform growth and palaeoceanographic change. In the French and Swiss Jura Mountains, the onset and evolution of the Urgonian platform have been controversially dated, and a correlation with other, better dated, successions is correspondingly difficult. It is for this reason that the stratigraphy and sedimentology of a series of recently exposed sections (Eclépens, Vaumarcus and Neuchâtel) and, in addition, the section of the Gorges de l’Areuse were analysed. Calcareous nannofossil biostratigraphy, the evolution of phosphorus contents of bulk rock, a sequence‐stratigraphic interpretation and a correlation of drowning unconformities with better dated sections in the Helvetic Alps were used to constrain the age of the Urgonian platform. The sum of the data and field observations suggests the following evolution: during the Hauterivian, important outward and upward growth of a bioclastic and oolitic carbonate platform is documented in two sequences, separated by a phase of platform drowning during the late Early Hauterivian. Following these two phases of platform growth, a second drowning phase occurred during the latest Hauterivian and Early Barremian, which was accompanied by significant platform erosion and sediment reworking. The Late Barremian witnessed the renewed installation of a carbonate platform, which initiated with a phase of oolite production, and which progressively evolved into a typical Urgonian carbonate platform colonized by corals and rudists. This phase terminated at the latest in the middle Early Aptian, due to a further drowning event. The evolution of this particular platform segment is compatible with that of more distal and well‐dated segments of the same northern Tethyan platform preserved in the Helvetic zone of the Alps and in the northern subalpine chains (Chartreuse and Vercors).  相似文献   

The incised valley of Baffin Bay,Texas: a tale of two climates     

ALEXANDER R. SIMMS  NIRANJAN ARYAL  LAUREN MILLER  YUSUKE YOKOYAMA 《Sedimentology》2010,57(2):642-669

Baffin Bay, Texas is the flooded Last Glacial Maximum incised valley of the Los Olmos, San Fernando and Petronila Creeks along the north‐western Gulf of Mexico. Cores up to 17 m in length and high‐resolution seismic profiles were used to study the history of Baffin Bay over the last 10 kyr and to document the unusual depositional environments within the valley fill. The deposits of the Baffin Bay incised valley record two major and two minor events. Around 8·0 ka, the estuarine environments backstepped more than 15 km in response to an increase in the rate of sea‐level rise. Around 5·5 ka, these estuarine environments changed from environments similar to other estuaries of the northern Gulf of Mexico to the unusual suite of environments found today. Another minor flooding event occurred around 4·8 ka in which several internal spits were flooded. Some time after 4·0 ka, the upper‐bay mud‐flats experienced a progradational event. Because of its semi‐arid climate and isolation from the Gulf of Mexico, five depositional environments not found in the other incised‐valley fills of the northern Gulf of Mexico are found today within Baffin Bay. These deposits include well‐laminated carbonate and siliciclastic open‐bay muds, ooid beaches, shelly internal spits and barrier islands, serpulid worm‐tube reefs and prograding upper‐bay mud‐flats. Based on these unusual deposits, and other characteristics of Baffin Bay, five criteria are suggested to help identify incised valleys that filled in arid and semi‐arid climates. These criteria include the presence of: (i) hypersaline‐tolerant fauna; (ii) aeolian deposits; and (iii) carbonate and/or evaporite deposits; and the absence of: (iv) peat or other organic‐rich deposits in the upper bay and bay‐margin areas; and (v) well‐developed fluvially dominated bayhead deltas.  相似文献   

哀牢山造山型金成矿系统:复合造山构造演化与成矿作用初探   总被引：55，自引：49，他引：6  

杨立强  刘江涛  张闯  王庆飞  葛良胜  王中亮  张静  龚庆杰 《岩石学报》2010,26(6):1723-1739

哀牢山金矿带是我国最重要的喜马拉雅期造山型金矿带,形成于三江特提斯复合造山过程中。论文基于对哀牢山复合造山带区域构造背景、控矿构造系统演化、金成矿期次及其时代的系统研究,从金成矿年代序列、成矿过程构造控制及成矿作用动力学环境三个方面,探讨了复合造山过程中的金矿成矿作用。研究结果表明,哀牢山金矿带发育三期金矿成矿-热事件:早期金成矿作用(61.55～63.09Ma)对应于逆冲推覆构造系统最为发育的时期,与剪切走滑断裂构造的形成同步,显示它们统一受控于印度-亚洲大陆碰撞早期的强烈汇聚挤压构造动力学体制;主期金成矿作用(33.76～36.10Ma)对应于区域挤压构造应力场的相对松弛阶段以及富碱斑岩和剪切走滑断裂构造系统最为发育的时期,受控于印度-亚洲大陆碰撞构造动力学转换体制,并可能受青藏高原物质东向逃逸和软流圈脉动隆起的联合制约,金矿大规模成矿作用与构造动力体制转换过程中的壳幔物质强烈交换与构造变形密切相关;晚期金成矿作用(26.40～30.80Ma)对应于岩石圈伸展作用的发生以及亏损地幔减压熔融产生的板内高钾岩浆岩的就位,受控于印度板块反向旋转拖曳与斜向俯冲回退的综合作用。  相似文献   

中国晚前寒武纪年表和年代地层序列   总被引：15，自引：3，他引：12       下载免费PDF全文

高林志  丁孝忠曹 茜 张传恒 《中国地质》2010,37(4):1014-1020

本文依据2009年11月24日全国地层委员会前寒武纪分会扩大会议上形成的一个共识,对中国晚前寒武纪年表进行重新标定:即长城系限定在1.8～1.6Ga,包括常州沟组、串岭沟组、团山子组、大红峪组;蓟县系限定在1.6～1.4Ga,包括高于庄组、杨庄组、雾迷山组、洪水庄组、铁岭组;待建系1.4～1.0Ga,蓟县剖面上仅发育下马岭组;青白口系限定在1.0～0.78Ga,包括骆驼岭组和景儿峪组;南华系限定在780～635Ma及震旦系限定在635～542Ma。关于最新的江南古陆晚前寒武纪地层中的一系列锆石U-Pb数据,应标定在青白口系上部。另外,华北古陆上最新的锆石U-Pb测年结果,初步揭示华北古陆前寒武系火山岩省的存在和分布范围,结合全球大陆动力学的基本特征,有利于我们建立一个前寒武纪统一的、精确的和具有年代系统的高精度年龄的基础剖面。  相似文献   

The exceptional Herbig Ae star HD 101412: The first detection of resolved magnetically split lines and the presence of chemical spots in a Herbig star     

S. Hubrig  M. Schller  I. Savanov  J.F. Gonzlez  C.R. Cowley  O. Schütz  R. Arlt  G. Rüdiger 《Astronomische Nachrichten》2010,331(4):361-367

In our previous search for magnetic fields in Herbig Ae stars, we pointed out that HD 101412 possesses the strongest magnetic field among the Herbig Ae stars and hence is of special interest for follow‐up studies of magnetism among young pre‐main‐sequence stars. We obtained high‐resolution, high signal‐to‐noise UVES and a few lower quality HARPS spectra revealing the presence of resolved magnetically split lines. HD 101412 is the first Herbig Ae star for which the rotational Doppler effect was found to be small in comparison to the magnetic splitting and several spectral lines observed in unpolarized light at high dispersion are resolved into magnetically split components. The measured mean magnetic field modulus varies from 2.5 to 3.5kG, while the mean quadratic field was found to vary in the range of 3.5 to 4.8 kG. To determine the period of variations, we used radial velocity, equivalent width, line width, and line asymmetry measurements of variable spectral lines of several elements, as well as magnetic field measurements. The period determination was done using the Lomb‐Scargle method. The most pronounced variability was detected for spectral lines of He I and the iron peak elements, whereas the spectral lines of CNO elements are only slightly variable. From spectral variations and magnetic field measurements we derived a potential rotation period P_rot = 13.86 d, which has to be proven in future studies with a larger number of observations. It is the first time that the presence of element spots is detected on the surface of a Herbig Ae/Be star. Our previous study of Herbig Ae stars revealed a trend towards stronger magnetic fields for younger Herbig Ae stars, confirmed by statistical tests. This is in contrast to a few other (non‐statistical) studies claiming that magnetic Herbig Ae stars are progenitors of the magnetic Ap stars. New developments in MHD theory show that the measured magnetic field strengths are compatible with a current‐driven instability of toroidal fields generated by differential rotation in the stellar interior. This explanation for magnetic intermediate‐mass stars could be an alternative to a frozen‐in fossil field (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

塔里木柯坪地区奥陶系层序地层与同位素地球化学响应特征   总被引：2，自引：0，他引：2  

胡明毅  钱勇  胡忠贵  王延奇  向娟 《岩石矿物学杂志》2010,29(2):199-205

塔里木盆地柯坪地区奥陶系发育浅水碳酸盐岩台地、深水陆棚-盆地两大类沉积体系和局限台地、开阔台地、陆棚和盆地等4种相类型。通过露头剖面的详细观察,在该区识别出局部暴露不整合和淹没不整合两类层序界面,以此为依据将该区奥陶系划分为9个三级层序。通过对层序格架内碳同位素和元素地球化学组成分析表明,不同层序界面及层序内不同体系域的δ13C和元素地球化学组成有明显的差异,并呈现出有规律性变化,反映出该区奥陶纪发生了多次海平面升降变化。研究表明同位素和地球化学特征可以作为层序地层学研究的辅助标志。  相似文献   

长庆白豹油田低渗透储层成岩作用及成岩储集相研究          下载免费PDF全文

王晓杰  彭仕宓  赵文光 《沉积与特提斯地质》2010,30(1):44-48

本文依据铸体薄片、电镜扫描、镜质体反射率、有机质成熟度等分析化验资料并结合岩石学特征,研究了长庆白豹油田长3、长4+5油层组的主要成岩作用,认为主要有压实作用、胶结作用、溶蚀作用和烃类侵位作用,而压溶作用不显著,总体上以破坏性成岩作用为主。总结了各成岩阶段的特征,建立了成岩演化序列。采用遗传神经网络算法求取成岩储集相参数,确定了A、B、C、D四种成岩储集相类型及其平面展布。  相似文献   

草鱼种质退化相关SRAP分子标记的筛选     

丁炜东曹丽萍  曹哲明 《广东海洋大学学报》2007,27(6):13-17

采用相关序列扩增多态性（sequence-reared amplified polymorphism，SRAP）技术分析野生草鱼和家养草鱼，并筛选与草鱼种质退化相关的分子遗传标记。共进行88对引物组合的检测，产生标记数目共计905个。依据标记在群体中出现的频率和变化规律，共筛选出21个可能与种质相关的特异性标记，对这些特异性标记进行测序并将测序结果进行BLAST分析，发现测得片段中有8个片段能在GeneBank中找到同源性较高的序列，而其他片段与数据库中序列的相似性较低。  相似文献   

湖北随州ML4.7地震序列基础资料分析     

李峰 李垠薛军蓉  陈俊华 《大地测量与地球动力学》2007,27(F06):56-61,88

依据随州三里岗ML4.7地震序列的地震监测和宏观调查所获得的基础资料,对此次地震序列的时空强特征及地震成因机理进行了分析。为使地震资料准确可靠,对混淆在序列中的爆破波形与地震波形进行了鉴别和剔除。结合这些基础资料和震源机制解结果。分析认为随州地震序列在成因上与该地区存在的北东和北西向两组断裂构造有关,但主发震构造是北西向断裂。  相似文献   

黑龙江东部区鸡西群、龙爪沟群时代与对比新认识     

姚淑荣  梁奉奎等 《中国煤田地质》2001,13(1):4-7,34

研究了鸡西，龙爪沟两群生物组合序列，重新划分了两群（组）的时代，并对两群对比关系提出了新认识。  相似文献