共查询到18条相似文献，搜索用时 890 毫秒
1.
贵阳乌当地区奥陶系湄潭组风暴岩特征 总被引：1，自引：0，他引：1
贵阳乌当地区奥陶系湄潭组下部的页岩中所夹的一层生物碎屑泥晶灰岩,是一个完整的风暴岩层,整个风暴岩厚约130cm,其沉积序列由下而上分为粒序段A、块段层段B、平行层理段C、丘状交错层理段D、小型沙纹层理段E以及泥岩段F,其A段+B段厚度小于D段+E段,为一下陆棚环境的远积风暴岩. 相似文献
2.
陕南川北志留系兰多维列统特列奇阶宁强组的生物礁 总被引：2，自引：0，他引：2
志留纪兰多维列世（Llandovery）扬子地台持续上升。特列奇期（Telychian）griestoniensis笔石带上部至spiralis-grandis带代表的时限内,地处扬子地台西北缘的宁强湾,在温暖浅海的环境中沉积了宁强组巨厚的泥页岩,其中夹含8套碳酸盐岩。在与之对应的8期小型局限碳酸盐岩台地的不同部位建造了生物礁和生物滩。生物礁的类型包括骨架礁、生物层和灰泥丘。生物礁群落由底栖固着的造礁珊瑚、苔藓虫、海百合、藻类、层孔虫,以及非固着的附礁生物腕足类、鹦鹉螺、三叶虫等组成。通过宁强广元地区不同地点和层位的生物礁组合分析,论述它们在生态组合、生长形状和发育过程中的多样性。 相似文献
3.
川西北广元-陕西宁强间下志留统巨厚的暗色泥岩地层中赋存有数以百计的生物礁，包括堤礁、点礁、堤状点礁群、生物岩丘、灰泥丘、层状岩丘，出露好，大小不一。礁是在浅水陆棚泥岩相的基础上发育起来的.造礁生物主要为横板珊瑚属的链珊瑚和蜂窝珊瑚及泡孔目的皮壳状、半球状苔藓虫。礁发育的基底主要为泥基质疙瘩状灰岩，也可以是生屑滩、近基风暴岩和淹没的潮坪层纹石灰岩。礁的衰亡以淹死型为主，少数为旱死型。在广元河湾场地区的河深１井钻遇礁组合５３.５５ｍ，中途测试有气浸显示、川南井下亦钻遇生物灰岩、生清灰岩（可能即为生物礁），见沥青充填裂隙、晶洞。包绕礁体的暗色泥岩有机炭丰度高。因之，志留系生物礁有希望成为四川盆地潜在的油气勘探目的层。 相似文献
4.
通过对红花生物礁露头的精细解剖和微相分析,研究了礁的内部构成和成礁模式。红花生物礁发育3期礁体旋回：礁A、礁B和礁C。礁A由生屑泥晶灰岩和骨架岩构成;礁B由生屑泥晶灰岩、粘结岩、骨架岩和生屑灰岩构成;礁C由粘结岩、骨架岩和生屑灰岩构成。红花生物礁造礁生物有钙质海绵、钙藻类、苔藓虫和水螅类,附礁生物为有孔虫、腕足类、双壳类、腹足类和棘皮动物等。单个礁体内,由下往上的生物演化为：腕足类+双壳类+有孔虫组合→钙藻类→钙质海绵+水螅类+钙藻类+苔藓虫组合→生物碎屑;岩性演化为：生屑泥晶灰岩→粘结岩→骨架岩→生屑灰岩。礁B的生屑滩内生屑间为泥晶充填,生屑分选、磨圆较好,是由相邻的高能生屑滩侵蚀搬运到礁B侧翼低能区沉积形成。3期礁都发育在碎屑滩上,礁A为低能环境下形成的礁,礁B和礁C在礁A形成的高地上成礁,为高能环境礁;单个礁体的完整成礁模式为：在浅滩之上,钙藻类大量生长、粘结吸附颗粒固结基底,钙质海绵和钙藻类在硬质基底上繁茂生长,形成具有抗浪格架的生物礁,礁体暴露水面死亡后遭波浪、水流改造形成生屑滩。 相似文献
5.
《现代地质》2016,(4)
生物礁是由原地的固着生物所建造的块状碳酸盐岩沉积。西沙海域自中新世以来发育了厚层生物礁地层。通过对最新全取心钻井西科1井岩心的宏观观察和微观分析,结合古生物及岩心测试成果,发现西科1井中新世和第四纪为主要造礁期,形成了两套分别以珊瑚藻和珊瑚为主要造礁生物的生物礁序列,底栖有孔虫为主要的附礁生物,而上新统为一套滩相沉积。生物礁序列发育骨架岩、粘结岩和障积岩三种礁相岩石,以骨架岩含量最高,非礁相岩石包括泥灰岩、颗粒灰岩和生物碎屑灰岩三种。白云岩地层以晚中新世到上新世早期最为发育,多为准同生白云石化作用所致,并受热液活动的影响。对生物礁序列的沉积分析,可为后期南海油气勘探以及生物礁储层分布研究提供一些基础材料。 相似文献
6.
鄂尔多斯盆地南部延长组长8-长6油层组沉积相为曲流河三角洲-半深湖、深湖,重力流沉积发育。以前认为这些重力流沉积物是浊流沉积。本文通过对旬邑地区延长组岩心、测井资料的研究,认为研究区长8-长6油层组发育砂质碎屑流沉积。岩心中常见大段块状砂岩、面状碎屑组构、顶底突变接触、漂砾、底部剪切带及滑塌变形构造等,相应测井曲线特征以箱型为主。砂质碎屑流为风暴诱因,可见丰富的风暴沉积特征,如侵蚀构造、底模、浪成沙纹层理、波痕、生物逃逸迹等。研究区理想的风暴沉积单元由下向上可概括为:块状层理段(A);滞留沉积段(B);平行层理段(C);丘状交错层理或浪成沙纹层理段(D);泥页岩段(E)。根据岩心风暴沉积特征总结出风暴岩的3个垂向沉积序列组合。砂质碎屑流及风暴作用的研究对于研究区油气勘探及古地理、古气候研究具有重要意义。 相似文献
7.
通过岩心观察,发现花港组典型的风暴沉积构造主要包括风暴侵蚀形成的渠模、冲刷沟槽、冲刷面,风暴涡流形成的撕扯构造、菊花状构造,风暴重力流形成的粒序层理,风暴浪形成的丘状交错层理、浪成沙纹层理、平行层理,同生变形构造及生物逃逸构造.运用岩石相组合分析的方法,发现花港组风暴垂向沉积序列发育不完整.其理想的序列由A~G共7段构成。根据花港组垂向沉积序列类型、沉积构造特点总结出了A+B+G、A+B+C、A+B+D、B+C+D、C+E+G、E+F+G等6种风暴沉积序列和原地风暴岩、近源风暴岩和远源风暴岩3种风暴岩类型. 相似文献
8.
川西北早志留世陆源碎屑──碳酸盐混积缓坡 总被引：10，自引：6，他引：10
研究区位于扬子地块西北缘，由一套巨厚的页岩、泥岩层夹生物礁及透镜状和不规则层状风暴生屑灰岩、瘤状灰岩组成。根据区内特征的岩石类型及其组合、分布和相应的化石生态，作者认为本区兰多维列期至早温洛克期时为一典型的陆源碎屑－－碳酸盐混积均斜缓坡，并且从浅到深划分为滨岸、浅缓坡、深缓坡及盆地等亚环境。滨岸区位于潮间带，以潮坪碳酸盐岩为代表；浅缓坡位于浪基面至风暴浪基面之间，岩性组合为Ａ、Ｂ类风暴岩，Ａ、Ｂ类瘤状灰岩、生物礁灰岩及粘结岩；深缓坡位于风暴浪基面至最大风暴浪基面之间，岩性以Ｄ、Ｅ类风暴岩、Ｃ类瘤状灰岩及泥页岩组合为特征；盆地处于最大风暴浪基面之下，为黑色泥页岩沉积。结合早志留世时全球冰川作用，文中讨论了海平面变化的原因及对环境的影响。 相似文献
9.
黔南罗甸沫阳剖面中二叠世茅口组以海相碳酸盐为主,下部地层中发育风暴岩,露头特征明显,主要以介壳灰岩为识别标志。风暴沉积构造包括底面侵蚀构造、截切构造、波痕层理、递变层理、块状层理等。风暴沉积主要包括一个底面构造A和B、C、D、E等四个沉积单元:A.侵蚀底面,代表风暴流对海底沉积物的作用;B.介壳灰岩层,代表风暴浪、风暴涡流沉积;C.粒序层,代表风暴衰减期重力分异沉积或风暴浊流沉积;D.块状层,代表风暴快速悬浮沉积;E.波痕层理段,代表风暴衰减后期沉积。它们共组成4种风暴沉积序列,分别代表不同深度的风暴沉积,反映了不同的风暴沉积作用和风暴流的类型。沫阳地区风暴沉积的沉积特征表明,该区风暴沉积主要发育于风暴浪基面之上的内陆棚沉积环境,风暴强度大,为近源风暴岩。仅个别风暴沉积发育于风暴浪基面之下的外陆棚沉积环境,为风暴引起的浊流沉积,为远源风暴岩。风暴岩类型的正确识别,对确定该区沉积相与深入认识扬子碳酸盐台地南部边缘沉积演化提供参考依据。 相似文献
10.
王家坪古杯礁丘是由不规则古杯和蓝绿藻Renalcis、Epiphyton、Cirvanella等组成的障积礁丘。可分为:孤立小型古杯泥丘和由丘状藻-古杯粘结岩叠置而成的点礁。以Renalcis为主的藻-古杯粘结岩与孤立小型古杯泥丘一样形成于风暴浪基面之下的低能陆架。以Epiphyton为主的藻-古杯粘结岩形成于较动荡的中-高能陆架浅滩。除造礁生物的沉积作用外,早期海底胶结作用和充填固化作用对古杯礁丘的形成亦起了十分重要的作用。 相似文献
11.
The 150–160 m thick lowermost Silurian (Rhuddanian) Becscie and Merrimack formations of Anticosti Island, Canada, represent continuous deposition on a shallow, open marine carbonate ramp. Several rock types are identified: (a) laminated and homogenous mudstone; (b) laminated and homogenous packstone; (c) argillaceous mudstone and packstone; (d) calcareous shale; (e) laminated calcisiltite; (f) medium- to fine-grained grainstone; and (g) bio/intraclastic rudstone. These rock types are arranged into five distinct lithofacies: (LF1) calcareous mudstone-shale; (LF2) laminated-homogenous mudstone; (LF3) calcareous grainstone-shale; (LF4) laminated mudstone-grainstone; and (LF5) laminated calcisiltite-grainstone. The sequence reflects deposition on a low-energy, muddy, carbonate to argillaceous ramp subject to short-lived, episodic high-energy storms. These events produced fining-upwards storm units 5–80 cm thick, or tempestites, consisting of: a sharp scoured base overlain by intra/bioclastic rudstone grading upwards into medium-grained grainstone, finely laminated calcisiltite and mudstone, or shale. These are interbedded with low-energy, fairweather mudstones and calcareous shales. Deposition progressed from a carbonate mud-dominated ramp in the Becscie Formation to an argillaceous mud-dominated ramp in the Merrimack Formation. Lateral tempestite proximality trends and lithofacies distribution indicate that the Anticosti Basin deepened to the south-east into the Iapetus Ocean and shallowed towards a SW—NE-orientated shoreline to the north-west. Vertical tempestite proximality trends and lithofacies changes identify third-order eustatic sea-level changes. After an initial deepening at the base of the formation, a shallowing-deepening event dominated the sequence. Several higher order fluctuations, defined by lithofacies and tempestite proximality trends, are superimposed on these changes. The fluctuations identified with the aid of tempestite proximality trends are of an order of magnitude higher than those identified by either lithofacies or palaeontological methods. 相似文献
12.
This study focuses on storm deposits in the Muschelkalk facies of the Betic Cordillera (southern Spain) and interprets their deposition mechanisms. Three types of storm deposit are distinguished: (i) pot/gutter casts; (ii) tempestite beds; and (iii) storm‐winnowed deposits. Each deposit provides information about the carbonate platform environment in which it was deposited. The tempestite models proposed are: (i) the bypass‐zone tempestite model, occurring in a muddy ramp at the epicontinental basin margin. This model is characterized by potholes and gutters that form in a shoreline bypass‐zone during storms; (ii) the gradient‐current tempestite model in which frequent tempestite beds are related to storm gradient currents. Thickness and grain size decrease towards the deep distal ramp; and (iii) the winnowed deposit tempestite model whereby storm deposits are winnowed and deposited in the same environment with only short lateral transport having occurred. This model evokes more restricted and shallower conditions, lagoons or inland seas. The distribution of all these deposits in the stratigraphic sections studied corroborate the eustatic third‐order cycle identified, although the different features of the storm deposits and their positions in each section indicate a subsidence varying in time and space. In the transgressive stage, the margins of the epicontinental basin were a well‐developed ramp with potholes and gutters. In contrast, during the high sea‐level stage, storm deposits generated tempestite beds or storm‐winnowed deposits in the different areas. The epicontinental carbonate platform with ramp edges evolved into a complex depositional system of coastal and shallow‐marine environments with lagoons and restricted inland seas. Thus, the epicontinental platform underwent substantial change from the Late Anisian to the Late Ladinian and this is reflected in its storm deposits. 相似文献
13.
本文在对湘中各地发现的下石炭统风暴岩的一般特征的讨论的基础上,区分出浅缓坡近源型、过渡带远源型以及深缓坡末梢型等风暴岩类型,并认为这些风暴岩的发育受当时全球古地理控制。早石炭世北方大陆和南方大陆之间存在的古地中海,造成了赤道附近飓风的形成条件。当时华南板块位于赤道以南接近赤道的地方,必然形成了大量风暴沉积。 相似文献
14.
川西北江油马角坝地区上石炭统黄龙组下部发育典型的风暴沉积,包括介壳灰岩、砾屑灰岩、瘤块状灰岩、砂屑灰岩和正常沉积灰岩或泥岩等沉积类型,以及冲刷沟槽、瘤块状构造、粒序层理、水平层理、波状层理和生物扰动等沉积构造。根据野外观察和室内显微分析,结合风暴沉积标志组合,在江油马角坝地区2个剖面的黄龙组下部各识别出4层风暴层,并划分出5套风暴沉积组合。组合Ⅰ以冲刷沟槽、介壳滞留层、粗砾滞留层、块状层理、水平层理、波状层理、泥灰岩层和生物富集层为特征,沉积于正常浪基面以上强风暴作用的开阔台地环境。组合Ⅱ以瘤块状构造、粒序层理和块状层理的生物碎屑灰岩为特征,沉积于正常浪基面之上受重力流影响的局限台地环境。组合Ⅲ以冲刷沟槽、粗砾滞留层、粒序层理、块状层理为特征,沉积于浪基面以上持续风暴流作用的开阔台地边缘浅滩环境。组合Ⅳ由冲刷沟槽、正粒序层理和块状层理的生物碎屑灰岩组成,产出于组合Ⅲ之上,表明该组合在前一期风暴未完全结束时又遭到后一期风暴的侵袭,接受浪基面之上的浅滩沉积。组合Ⅴ由冲刷沟槽、粗砾滞留层和泥岩层组成,沉积于晴天浪基面以上缺少物源的极浅水开阔台地环境。以上5种组合风暴岩都发育于台地中上部,与一般的斜坡风暴岩有明显的差别,均属于近源极浅水风暴岩。风暴岩的研究对地层对比、古气候、岩相古地理、沉积盆地演化和油气勘探具有重要的理论和现实意义。 相似文献
15.
LEE Jeong-Hyun KIM Byeong-Jun LIANG Kun PARK Tae-Yoon S. CHOH Suk-Joo LEE Dong-Jin WOO Jusun 《《地质学报》英文版》2016,90(6):1946-1954
Mid to late Cambrian thrombolites and maze-like maceriate reefs from the western North China Platform, Wuhai, Inner Mongolia, northwestern China, occur in the middle of a succession dominated by thin-bedded lime mudstone-shale/marlstone alternations, and are laterally surrounded by limestone conglomerate and/or grainstone. Thrombolite, characterized by meter-scale lenticular mounds composed of millimeter- to centimeter-scale mesoclots and wackestone matrix, occurs in the lower middle part of the sequence. Thrombolite mesoclots are composed of microstromatolites with alternating dark gray and light gray micritic laminae. The maze-like maceriate reefs occur in the middle to the upper part of the sequence, commonly forming lenticular mounds up to 1 m thick. They are characterized by centimeter- to decimeter-scale branched maze-like structures, whose biogenic portions (maceria) are selectively dolomitized. The maceriae are composed of poorly preserved microstromatolites and siliceous sponges. Inter-macerial sediments consist of lime mud and scattered bioclasts. These Wuhai reefs are generally similar to but older than various other Cambrian reefs previously reported from the Shandong region, northeastern China. 相似文献
16.
Isolated, high relief carbonate platforms developed in the intracratonic basin of east-central Mexico during Albian-Cenomanian time. Relief on the platforms was of the order of 1000 m and slopes were as steep as 20–43°. Basin-margin debris aprons adjacent to the platforms comprise the Tamabra Formation. In the Sierra Madre Oriental, at the eastern margin of the Valles-San Luis Potosi Platform, an exceptionally thick (1380m) progradational basin to platform sequence of the Tamabra Formation can be divided into six lithological units. Basinal carbonate deposition that preceded deposition of the Tamabra Formation was emphatically punctuated by an allochthonous reef block 1 km long by 0·5 km wide with a stratigraphic thickness of 95 m. It is encased in Tamabra Formation unit A, approximately 360 m of peloidal-skeletal wackestone and lithoclastic-skeletal packstone that includes some graded beds. Unit B is 73 m of massive dolomite with sparse skeletal fragments and intraclasts. Unit C, 114m thick, consists of structureless skeletal wackestone passing upward into graded skeletal packstone. Interlaminated lime mudstone and fine grained bioclastic packstone with prominent horizontal burrows are interspersed near the top. Unit D is 126 m of breccia with finely interbedded skeletal grainstone and burrowed or laminated mudstone. The breccias contain a spectrum of platform-derived lithoclasts and basinal intraclasts, up to 10 m in size. The breccias are typically grain supported (rudstone) with a matrix of lightly to completely dolomitized mudstone or skeletal debris. Beds are up to several metres thick. Unit E is 206 m of massive, sucrosic dolomite that replaced breccias. Unit F is approximately 500 m of thick bedded to massive skeletal packstone with abundant rudists and a few mudstone intraclasts. Metre scale laminated lime mudstone beds are interspersed. The section is capped by El Abra Formation platform margin limestone, consisting of massive beds of caprinid packstone and grainstone with many whole valves. Depositional processes within this sequence shift from basinal pelagic or peri-platform sedimentation to distal, platform-derived, muddy turbidity currents with a large slump block (Unit A); through more proximal (coarser and cleaner) turbidity currents (Unit B?, C); to debris flows incorporating platform margin and slope debris (Units D, E). Finally, a talus of coarse, reef-derived bioclasts (Unit F) accumulated as the platform margin prograded over the slope sequence. Interspersed basinal deposits evolved gradually from largely pelagic to include influxes of dilute turbidity currents. Units containing turbidites with platform-derived bioclasts reflect flooding of the adjacent platform. Breccia blocks and lithoclasts were probably generated by erosion and collapse of the platform during lowstands. Laminated, black, pelagic carbonates, locally cherty, are interbedded with both breccias and turbidites. At least those interbedded with turbidites may have been deposited within an expanded mid-water oxygen minimum zone during relative highstands of sea level. They are in part coeval with mid-Cretaceous black shales of the Atlantic Ocean. 相似文献
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焦凤辰 《沉积与特提斯地质》1988,8(6):38-42
四川省会理县洪川桥地区,是会理群凤山营组广泛分布地区之一,出露面积达百余平方公里。在洪川桥凤山营组剖面的上部(洪剖119层—108层),发育一套约845m厚的风暴流沉积。现将其特征及形成机制作一初步分析,以供参考。一、岩性特征风暴流沉积物,主要为灰—深灰色粉砂质粉屑灰岩和部分泥质灰岩。有时两者呈薄的互层出现。一般层厚几毫米到几厘米,沿走向在数十厘米或几米内尖灭,形成一个个薄的透镜 相似文献