辽东本溪林家组属于中三叠世之锆石、古生物和地层证据     

张宜  郑少林  李之彤  曹成润  杨佳林  张国仁  李显东  孟繁巍 《地质与资源》2019,28(5):434-442

林家组出露于辽宁东部本溪林家崴子一带.自小林贞一1942年记载以来，其时代一直有很大的争议.争议跨度从第三系到上二叠统.20世纪80年代初，张武等依据动植物化石和地层对比，提出了林家组属于中三叠世的观点.由于林家组产出的植物化石十分复杂，既有古生代，又有中生代分子，且没有锆石年龄证据，故林家组时代仍然存疑.近年来，在林家组底部找到了变质凝灰质粉砂岩，其中有很多锆石.根据30颗保存较好锆石测年结果，发现4颗最年轻锆石的²⁰⁶Pb/²³⁸U平均年龄是239.5±4.1 Ma.另外，最近前甸子地区林家组发现了少林肋木（Pleuromeia shaolinii）.因此尽管林家植物群存在二叠纪和三叠纪均有分布的重要植物，但结合锆石定年、地层对比、岩性特征、平行不整合接触关系、三叠纪代表植物及中三叠世到早白垩世均有分布的昆虫索德蠊属来综合分析，可以确认林家组确实属于中三叠世.  相似文献   

An Automatic Method for Detecting Transients and Variable Sources in AST3 Survey Based on Image Subtraction and Random Forest     

《Chinese Astronomy and Astrophysics》2020,44(1):41-60

AST3-2 (the second Antarctic Survey Telescope) is located in Antarctic Dome A, the loftiest ice dome on the Antarctic Plateau. It produces a huge amount of observational data which require a more efficient data reduction program to be developed. Also the data transmission in Antarctica is much difficult, thus it is necessary to perform data reduction and detect variable and transient sources remotely and automatically in Antarctica, but this attempt is restricted by the unsatisfactory performance of the low power consumption computer in Antarctica. For realizing this purpose, to develop a new method based on the existing image subtraction method and random forest algorithm, taking the AST3-2 2016 dataset as the test sample, becomes an alternative choice. This method performs image subtraction on the dataset, then applies the principle component analysis to extract the features of residual images. Random forest is used as a machine learning classifier, and in the test a recall rate of 97% is resulted for the positive sample. Our work has verified the feasibility and accuracy of this method, and finally found out a batch of candidates for variable stars in the AST3-2 2016 dataset.  相似文献   

鄂尔多斯盆地塔然高勒地区直罗组上、下段的岩性-岩相特征及对铀成矿的差异性控制作用     

朱强  李建国  俞礽安  司马献章  文思博  李光耀  司庆红 《地球学报》2019,40(3):456-468

为查明鄂尔多斯盆地塔然高勒地区直罗组上段、下段的岩性-岩相特征以及参与蚀变作用的流体强度差异,开展了系统的岩心观察、剖面对比,并结合黏土矿物、碳氧同位素和U、Th元素等手段进行分析。结果表明,研究区南部直罗组上段主要由灰绿色、红色泥岩夹透镜状红色、黄色、灰绿色砂岩组成,北部主要由红色泥岩与灰绿色砂岩构成,南北部下段均由灰白色、灰绿色砂岩或砂砾岩夹薄层泥岩组成。直罗组红色砂岩为原生沉积,灰绿色砂岩为后生改造类型;上段受含氧含铀水和深部还原性流体作用强度较下段变弱,且由北向南作用程度降低,北部还原蚀变岩石与原生岩石共存,南部基本保留原生岩石;下段则受流体改造更为充分,主体为后生蚀变岩石。直罗组不同类型砂体的展布兼受沉积相和后期流体双重作用,但强弱差异性明显,限制了铀矿化产出在直罗组下段砂体中的定位,因此,上、下段应作为不同的成矿体系讨论。  相似文献   

古/中元古代界线:1.8Ga   总被引：1，自引：0，他引：1  

赵太平  庞岚尹  仇一凡  祝禧艳  王世炎  耿元生 《岩石学报》2019,35(8):2281-2298

年代地层表是我们描述地球历史演化的时间框架,也隐含着我们对地球演化过程的基本认识,承载着一系列核心科学问题。现有的国际前寒武纪地质年表存在不少问题,还没有被普遍接受的新方案。在现行国际地层年表(IUGS 1989—2004)中,20～18亿年被称为造山纪,18～16亿年被称为固结纪,16～14亿年被称为盖层纪,也即:造山运动结束到盖层发育之间的过渡时期为固结纪,而将盖层的广泛发育作为中元古代的开始。在我国,由于"吕梁运动"是华北克拉通结晶基底最终形成的标志性构造-热事件,此后发育以长城系-蓟县系-青白口系为代表的地台型沉积盖层,因此我国地质界一直以长城系的底界代表中元古代的开始,并根据"吕梁运动"结束时间,将古/中元古代的时间界线置于18亿年。2012年国际地层委员会提出了一份全新的全球前寒武纪地质年代表划分建议方案,其中2060～1780Ma阶段被称为古元古代哥伦比亚纪,主要以Columbia超大陆的聚合为特征;而之后17. 8～8. 5亿年的近10亿年间,则被定义为罗迪尼亚纪,代表了从Columbia超大陆裂解到Rodinia超大陆聚合的漫长阶段。即这一新建议方案的古/中元古代界线为17. 8亿年,与我国学者长期以来所坚持的古/中元古代分界是基本一致的。在华北克拉通,"吕梁运动"的结束时间在～18亿年,此后整体处于多期裂解的陆内伸展环境,长城系-蓟县系基本上属于连续的陆表海沉积。近年来的研究表明,燕山地区长城系的底界年龄约为17亿年,长城系与蓟县系的分界则为16亿年。如果一味按照现行国际地层划分方案,其古/中元古代的界线(16亿年)将对应于长城系-蓟县系的分界,华北克拉通这套盖层型沉积将被人为分割为两部分,这显然是很不合理的。值得注意的是,在华北克拉通中部吕梁地区发育的小两岭组火山岩和在其南部地区发育的、也是世界范围内同时期最大规模的火山活动——熊耳群火山-沉积岩系,是华北克拉通结晶基底之上最早发育的盖层沉积,其起始形成时间约为18亿年。这与新建议的古/中元古代分界非常接近。从全球地质演化来看,从18到16亿年,造山作用结束,Columbia超大陆开始裂解,岩浆作用方式和岩浆岩组合类型及其地球化学特征发生明显改变,如斜长岩、环斑花岗岩在世界主要克拉通均有发育。与此同时,稳定沉积盖层开始广泛发育,条带状铁建造(BIF)消失,代之以鲕状或粒状矿物集合体组成的浅海富铁沉积,另外海相硫化物沉积、有核原生生物等也首次出现。所有这些都标志着,在此前后,地球岩石圈、水圈和大气圈均发生了重大转折,生物圈也进入新的演化阶段,标志着地球进入"中年期"演化阶段。虽然地球演化发生重要转折的根本原因和细节还有待进一步深入探讨,但这一转变的起点或最重要的时间点,无疑就在18亿年前后,因此,本文认为,应将其作为全球古/中元古代的时间界线。  相似文献   

Research on Parallel Algorithms for uv-faceting Imaging     

《Chinese Astronomy and Astrophysics》2019,43(3):424-443

The uv-faceting imaging is one of the widely used large field of view imaging technologies, and will be adopted for the data processing of the low-frequency array in the first stage of the Square Kilometre Array (SKA1). Due to the scale of the raw data of SKA1 is unprecedentedly large, the efficiency of data processing directly using the original uv-faceting imaging will be very low. Therefore, a uv-faceting imaging algorithm based on the MPI (Message Passing Interface)+OpenMP (Open Multi-Processing) and a uv-faceting imaging algorithm based on the MPI+CUDA (Compute Unified Device Architecture) are proposed. The most time-consuming data reading and gridding in the algorithm are optimized in parallel. The verification results show that the results of the proposed two algorithms are basically consistent with that obtained by the current mainstream data processing software CASA (Common Astronomy Software Applications), which indicates that the proposed two algorithms are basically correct. Further analysis of the accuracy and total running time shows that the MPI+CUDA method is better than the MPI+OpenMP method in both the correctness rate and running speed. The performance test results show that the proposed algorithms are effective and have certain extensibility.  相似文献   

Study of Star/Galaxy Classification Based on the XGBoost Algorithm     

《Chinese Astronomy and Astrophysics》2019,43(4):539-548

Machine learning has achieved great success in many areas today. The lifting algorithm has a strong ability to adapt to various scenarios with a high accuracy, and has played a great role in many fields. But in astronomy, the application of lifting algorithms is still rare. In response to the low classification accuracy of the dark star/galaxy source set in the Sloan Digital Sky Survey (SDSS), a new research result of machine learning, eXtreme Gradient Boosting (XGBoost), has been introduced. The complete photometric data set is obtained from the SDSS-DR7, and divided into a bright source set and a dark source set according to the star magnitude. Firstly, the ten-fold cross-validation method is used for the bright source set and the dark source set respectively, and the XGBoost algorithm is used to establish the star/galaxy classification model. Then, the grid search and other methods are used to adjust the XGBoost parameters. Finally, based on the galaxy classification accuracy and other indicators, the classification results are analyzed, by comparing with the models of function tree (FT), Adaptive boosting (Adaboost), Random Forest (RF), Gradient Boosting Decision Tree (GBDT), Stacked Denoising AutoEncoders (SDAE), and Deep Belief Nets (DBN). The experimental results show that, the XGBoost improves the classification accuracy of galaxies in the dark source classification by nearly 10% as compared to the function tree algorithm, and improves the classification accuracy of sources with the darkest magnitudes in the dark source set by nearly 5% as compared to the function tree algorithm. Compared with other traditional machine learning algorithms and deep neural networks, the XGBoost also has different degrees of improvement.  相似文献   

Nanpanjiang basin: A window on the tectonic development of south China during Triassic assembly of the southeastern and eastern Asia     

《Gondwana Research》2020

As the largest siliciclastic sink in the South China block, the Triassic Nanpanjiang basin is generally thought of as a foreland basin related to Indosinian collision between the South China and Indochina blocks. Our basin analysis, spanning an eight years period, provides details of Lopingian to Middle Triassic stratigraphic fill and tectonic subsidence of the basin. Field observation and sedimentological analyses reveal that the basin was not filled by a monotonous turbidite system and suggest instead the development of five primary depositional units constituted by deep-water turbidite systems, mass-transport deposits, condensed drapes, shallow-water isolated carbonate platforms, and volcano-volcaniclastic rocks. The stratigraphic completeness of the basin, the coexistence of widespread but localized carbonate platforms within axially filled deep-water basin, tectonically generated cyclothems of transverse mass-transport deposits along intrabasinal faults and basin fill of extrusive rocks of bimodal composition together apparently call in question the claim that crustal shortening prevailed during the Late Permian to pre-Norian Triassic. Patterns of basin fill, differential tectonic subsidence and very high subsidence rate of the region adjacent to master fault are more closely match the pattern expected for extensional to transtensional basin in a back-arc setting. The crustal extension in the southwestern South China was not consistent with hypothesized Indosinian collision between South China and Indochina blocks, but more likely developed in response to northwestward subduction of the paleo-Pacific plate. Our results, combined with regional considerations, lead to a new model for the Triassic tectonic evolution of South China during Triassic assembly of the southeastern and eastern Asia.  相似文献   

Tectono-sedimentary evolution of Jurassic–Cretaceous diapiric structures: Miravete anticline,Maestrat Basin,Spain     

Jaume Vergés  Yohann Poprawski  Ylènia Almar  Peter A. Drzewiecki  Mar Moragas  Telm Bover-Arnal  Chiara Macchiavelli  Wayne Wright  Grégoire Messager  Jean-Christophe Embry  David Hunt 《Basin Research》2020,32(6):1653-1684

Integration of extensive fieldwork, remote sensing mapping and 3D models from high-quality drone photographs relates tectonics and sedimentation to define the Jurassic–early Albian diapiric evolution of the N–S Miravete anticline, the NW-SE Castel de Cabra anticline and the NW-SE Cañada Vellida ridge in the Maestrat Basin (Iberian Ranges, Spain). The pre shortening diapiric structures are defined by well-exposed and unambiguous halokinetic geometries such as hooks and flaps, salt walls and collapse normal faults. These were developed on Triassic salt-bearing deposits, previously misinterpreted because they were hidden and overprinted by the Alpine shortening. The Miravete anticline grew during the Jurassic and Early Cretaceous and was rejuvenated during Cenozoic shortening. Its evolution is separated into four halokinetic stages, including the latest Alpine compression. Regionally, the well-exposed Castel de Cabra salt anticline and Cañada Vellida salt wall confirm the widespread Jurassic and Early Cretaceous diapiric evolution of the Maestrat Basin. The NE flank of the Cañada Vellida salt wall is characterized by hook patterns and by a 500-m-long thin Upper Jurassic carbonates defining an upturned flap, inferred as the roof of the salt wall before NE-directed salt extrusion. A regional E-W cross section through the Ababuj, Miravete and Cañada-Benatanduz anticlines shows typical geometries of salt-related rift basins, partly decoupled from basement faults. These structures could form a broader diapiric region still to be investigated. In this section, the Camarillas and Fortanete minibasins displayed well-developed bowl geometries at the onset of shortening. The most active period of diapiric growth in the Maestrat Basin occurred during the Early Cretaceous, which is also recorded in the Eastern Betics, Asturias and Basque-Cantabrian basins. This period coincides with the peak of eastward drift of the Iberian microplate, with speeds of 20 mm/year. The transtensional regime is interpreted to have played a role in diapiric development.  相似文献   

松辽盆地东北缘白垩系砂岩型铀矿成矿条件与找矿方向     

代问义  李研  赵忠华  张杨  张航 《地质与资源》2019,28(6):519

通过松辽盆地东北缘蚀源区铀源条件、中生代构造演化、白垩系沉积建造研究，结合石油部门地震连井剖面等资料，综合分析了松辽盆地东北部砂岩型铀矿的成矿条件研究，认为盆缘的富铀花岗岩体提供了丰富的铀源，中生代后期反转构造形成的剥蚀天窗为含铀含氧水的渗入渗出提供了通道.研究结果显示，松辽盆地东北部绥棱地区为最有利的砂岩型铀矿找矿部位，主要找矿目标层为上白垩统泉头组兼顾浅部姚家组，找矿类型为层间氧化带型.  相似文献   

华南上扬子区深部温度估算及其油气地质意义     

李香兰  刘绍文  徐明  李旭东  郝春艳 《地质学报》2020,94(6):1896-1910

盆地热体制及深部温度估算对油气和区域地热能资源评估具有重要意义。南方上扬子区是海相油气勘探的重要区块,近年来更是我国页岩气勘探的主要选区。然而,由于数据不足及研究目标的分散,该区的盆地热体制特征还有待深化。结合前人已有地热数据,并整合新近开展的稳态测温数据,我们揭示了上扬子区现今地温梯度、大地热流分布特征,继而估算了1000～6000m埋深处的深部地层温度和2套主要古生界海相烃源岩底界面处的温度。结果表明,上扬子区具有中-低温的地热状态,其现今地温梯度和大地热流的范围(平均值)分别为10～74℃/km(24℃/km)和27～118mW/m~2(64mW/m~2),整体上从东北向西南方向递增,呈现出"东北低、西南高"的分布趋势。1000～6000m埋深处估算温度的分布格局与地温梯度及热流的分布趋势基本一致。东北部的鄂西-湘北地区为低温区,中部的四川盆地其大部分为中温区,西南的云南地区为高温区。上扬子区现今地热分布格局受区域差异构造和岩浆作用控制。结合储层温度估算并综合其他油气地质资料,提出川东的石柱-涪陵、川南的威远-自贡-泸州和宜宾-长宁等区的下志留统龙马溪组页岩层系是上扬子区油气勘探有利区带。  相似文献