福建建宁均口地区早白垩世火山地质特征     

李金秋 《福建地质》1996,15(2):71-90

建宁均口地区早白垩世火山岩可划分为２个组４个段，火山岩双峰式组合特征明显，火山岩相特征及空间分布特征显著，区内发现７个火山机构和２个寄生火山，安远－都畲线状火山群由５个受裂隙控制的中心式火山机构所组成，是寻找金矿和非金属矿的有利部位，火山活动的构造环境为拉张环境；岩浆来源可能源于地壳和上地幔。  相似文献   

新地球动力学模式的探讨     

吴友林  林舸 《华东地质学院学报》1996,19(1):7-13

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民和盆地巴州坳陷中侏罗─下白垩统沉积相序列及其含油气意义   总被引：1，自引：0，他引：1  

邓涛 《西北地质科学》1996,(2)

民和盆地巴州坳陷的侏罗－下白垩统主要发育曲流河、辫状河、滨浅湖、水下扇和三角洲沉积。窑街组的漫滩沼泽和湖湾沉积是主要的生油岩系。享堂组、大通河组和河口组的河道砂坝、湖滩滩砂和水下扇水道砂体是主要的储集层．其中，河道砂坝是最重要的。由于受成岩作用影响，孔隙度和渗透率都较低，裂缝－溶蚀孔隙改善了储层的储集性能。根据沉积特征，提出滨浅湖砂滩和水下扇水道是值得注意的有利储集相带。中侏罗统以上的滨浅湖泥岩和粉砂质泥岩是主要的盖层。  相似文献   

略论泰州组及其时代   总被引：1，自引：2，他引：1  

张一勇 《地层学杂志》1996,20(1):45-50

利用孢粉系统学方法研究前人发表的江苏北部海安凹陷和盆地西缘钦30井泰州组的孢粉组合,并由此对这两个地区泰州组的地质年代和区域对比提出不同的看法:即海安凹陷的泰州组应是白垩纪最晚的马斯特里赫特期的沉积,而钦30井泰州组则为坎佩尼或部分为前坎佩尼期的沉积。结合介形类动物群的产出,将上述两地区的泰州组与泰州组建组的泰1井泰州组等进行了对比。  相似文献   

松辽盆地白垩系青山口组黑色页岩的形成环境及海水侵入的底流模式   总被引：6，自引：0，他引：6       下载免费PDF全文

王璞珺  王东坡  杜小弟 《沉积与特提斯地质》1996,16(1):34-43

通过对中央坳陷区两口钻井剖面和东南隆起区野外露头剖面的沉积学、矿物学和地球化学研究，认为松辽盆地白垩系青山口组黑色页岩形成于稳定分层的湖相环境；周期性海水注入形成的底流是导致水体分层和黑色页岩沉积的重要因素。  相似文献   

周口坳陷早白垩世沉积相与沉积格局   总被引：1，自引：0，他引：1       下载免费PDF全文

李文厚  陈景维  邵磊 《沉积与特提斯地质》1996,16(1):44-50

周口坳陷早白垩世主要发育冲积扇相、河流相、湖泊相、扇三角洲相和三角洲相等类型，其中谭庄－沈丘凹陷沉积相带呈东西向狭长展布，是一个典型的断陷盆地．本文在讨论了湖盆的物源、古地形、古水流、水介质条件及古气候条件的基础上，提出了早白垩世时周口坳陷的沉积格局。  相似文献   

中国中东部白垩纪沙漠的时空分布及其气候意义   总被引：6，自引：3，他引：6       下载免费PDF全文

江新胜  李玉文 《沉积与特提斯地质》1996,16(2):42-51

本文介绍了中国中东部白垩纪沙漠沉积的时空分布，探讨了时空分布规律，认为：（１）中东部白垩纪沙漠分布严格受气候带控制，其实际分布限于北纬２０—４０°的干旱带（横跨当时的副热高压带），主要分布于鄂尔多斯盆地、四川盆地、江汉盆地和苏北盆地之中；（２）各盆地沙漠发生的时间不同，鄂尔多斯盆地为早白垩世，四川盆地为中白垩世晚期，江汉盆地为晚白垩世早期，苏北盆地为晚白垩世中期，（３）沙漠发生的穿时性反映了各盆地进入干旱带的顺序，由北到南，由西及东；（４）造成这种顺序的原因是由于亚洲在白垩纪时其总体为顺时针旋转，因而使西北部鄂尔多斯盆地率先进入干旱带，其次是西南部的四川盆地，然后是中部的江汉盆地。晚白垩世的降温事件迫使干旱带南移而使其滞后的最东部的苏北盆地进入干旱带，（５）中国白垩纪沙漠的存在说明处于“温室效应”的大气环流不仅不会“呆滞”而且还有所增强，季风的存在也说明当时的气候并不均一。本文提出了气候带漂变（ｃｌｉｍａｔｉｃｚｏｎｅｄｒｉｆｔ）的概念，认为气候变化的表现形式为气候带漂变。漂变既有长周期和短周期漂变之分，又有相对和绝对漂变之别。中国中东部白垩纪沙漠的时空变迁就是干旱气候带漂变的结果。  相似文献   

Re-evaluation of the phylogeny of Early Cretaceous planktonic foraminifera (Praehedbergellidae)     

Marcelle K. BouDagher-Fadel 《Cretaceous Research》1996,17(6):767-771

Tunisia, Ukraine, Russia, the North Sea area and elsewhere have yielded knowledge that the Early Cretaceous planktonic foraminifera are predominantly members of the Praehedbergellidae. The taxonomy and phylogeny of this family have been revised and refined. New generic and specific taxa have been proposed, new phylogenetic lineages have been described, and many type specimens have been imaged by scanning electron microscopy for the first time.Gorbachikella(Hauterivian–Early Aptian) gave rise toPraehedbergella(Late Hauterivian–Late Aptian), evolvingBlefuscuiana,Lilliputianella, and the planospiralBlowiellain the Barremian. The last gave rise toGlobigerinelloidesin the Aptian, from which the macroperforateAlanlordella(and its descendantPlanomalina) evolved in the Albian.Blowiellawas ancestral to taxa with radially elongated chambers (Claviblowiella, Leupoldina, Schackoina).  相似文献   

Cretaceous episodic growth of the Japanese Islands   总被引：1，自引：0，他引：1  

G. Kimura 《Island Arc》1997,6(1):52-68

Abstract The Japanese Islands formed rapidly in situ along the eastern Asian continental margin in the Cretaceous due to both tectonic and magmatic processes. In the Early Cretaceous, huge oceanic plateaus created by the mid-Panthalassa super plume accreted with the continental margin. This tectonic interaction of oceanic plateau with continental crust is one of the significant tectonic processes responsible for continental growth in subduction zones. In the Japanese Islands, Late Cretaceous-Early Paleogene continental growth is much more episodic and drastic. At this time the continental margin uplifted regionally, and intra-continent collision tectonics took place in the northern part of the Asian continent. The uplifting event appears to have been caused by the subduction of very young oceanic crust (i.e. the Izanagi-Kula Plate) along the continental margin. Magmatism was also very active, and melting of the young oceanic slab appears to have resulted in ubiquitous plutons in the continental margin. Regional uplift of the continental margin and intra-continent collision tectonics promoted erosion of the uplifted area, and a large amount of terrigenous sediment was abruptly supplied to the trench. As a result of the rapid supply of terrigenous detritus, the accretionary complexes (the Hidaka Belt in Hokkaido and the Shimanto Belt in Southwest Japan) grew rapidly in the subduction zone. The rapid growth of the accretionary complexes and the subduction of very young, buoyant oceanic crust caused the extrusion of a high-P/T metamorphic wedge from the deep levels of the subduction zone. Episodic growth of the Late Cretaceous Japanese Islands suggests that subduction of very young oceanic crust and/or ridge subduction are very significant for the formation of new continental crust in subduction zones.  相似文献   

Subduction influence on magma supply at the East Scotia Ridge     

Roy Livermore  Alex Cunningham  Lieve Vanneste  Robert Larter 《Earth and Planetary Science Letters》1997,150(3-4):261-275

Despite a spreading rate of 65–70 km Ma⁻¹, the East Scotia Ridge has, along most of its length, a form typically associated with slower rates of sea floor spreading. This may be a consequence of cooler than normal mantle upwelling, which could be a feature of back-arc spreading. At the northern end of the ridge, recently acquired sonar data show a complex, rapidly evolving pattern of extension within 100 km of the South Sandwich Trench. New ridge segments appear to be nucleating at or near the boundary between the South American and Scotia Sea plates and propagating southwards, supplanting older segments. The most prominent of these, north of 56°30′S, has been propagating at a rate of approximately 60 km Ma⁻¹ for at least 1 Ma, and displays a morphology unique on this plate boundary. A 40 km long axial high exists at the centre of this segment, forming one of the shallowest sections of the East Scotia Ridge. Beneath it, seismic reflection profiles reveal an axial magma chamber, or AMC, reflector, similar to those observed beneath the East Pacific Rise and Valu Fa Ridge. Simple calculations indicate the existence here of a narrow (<1 km wide) body of melt at a depth of approximately 3 km beneath the sea floor. From the topographic and seismic data, we deduce that a localised mantle melting anomaly lies beneath this segment. Rates of spreading in the east Scotia Sea show little variation along axis. Hence, the changes in melt supply are related to the unique tectonic setting, in which the South American plate is tearing to the east, perhaps allowing mantle flow around the end of the subducting slab. Volatiles released from the torn plate edge and entrained in the flow are a potential cause of the anomalous melting observed. A southward mantle flow may have existed beneath the axis of the East Scotia Ridge throughout its history.  相似文献