Protoconodont fossils for refining the Cambrian bottom and the contribution to shale gas formation along the southwest margin of Yangtze Block     

《China Geology》2020,3(4):558-566

It has been an intense debate on the exact boundary between Ediacaran and Cambrian in the southwest Yangtze Block. The calibration of this critical boundary has a remarkable influence on the further investigation of the break-up of the Rodinia Supercontinent, the early life evolution, and the mechanism of the phosphorite deposit. Ediacaran and Cambrian strata and fossils are widely distributed in Anning, Yunnan Province in China. In recent years, the Xiaowaitoushan Member from the Lower Yuhucun Formation has been studied. Through this interval with continuous collections, the first appearance datums (FADs) of the protoconodont (Fomitchella cf. inchoate Yang et He, Protohertzina cf. anabarica Missarzhevsky) and globular embryos fossil (Olivooides sp.) earlier than these in the Lower Cambrian strata of the Meishucun Formation were discovered. This discovery indicates that the Xiaowaitoushan Member has included more FADs than the previously discovered single FAD of Anabarites primitivus Qian et Jiang, and the Ediacaran–Cambrian boundary in southwest China should be replaced below the Point “A” of the Meishucun Formation in Yunnan Province. The Point “B” of the Meishucun Formation is younger than the suggested age 541 Ma of the Ediacaran–Cambrian boundary and can no longer reference the Global Boundary Stratotype Section and Point (GSSP) correlation in southwest China. It can be suggested based on the previous stratigraphy and palaeontology studies from northern Sichuan and southern Shaanxi and the FAD of the globular embryos fossils that the Ediacaran−Cambrian boundary in the southwest Yangtze Block should be placed at the base of the Xiaowaitoushan Member; other phosphorite strata refer to Xiaowaitoushan Member. The discovery of the FADs of the shelly fossils in the Xiaowaitoushan Member provides new evidence for the global correlation of the Ediacaran –Cambrian boundary in the southwest Yangtze Block. The conodont discoloration index (CAI) of the specimens in Anning is between 2 and 3, which indicates that the organic matter in Xiaowaitoushan Member is matured and has high potential to form a shale gas reservoir.  相似文献   

老挝万象地区基础地质调研的主要进展   总被引：9，自引：0，他引：9  

严城民  朱延浙  吴军  冯明刚 《地球学报》2006,27(1):81-84

经区域地质调查、专题研究及钻探工程,老挝万象地区基础地质调研取得的主要进展是:①该区地层自下而上可划分为会辛南组(P2HX)、南拉组(P2NL)、南康尚组(P2NK)、南立组(J1NL)、南舍组(J1-2NS)、班辛黑组(J2BH)、普帕纳帕陶山组(K1PP)、班纳德组(K1BN)、班塔拉组(K1BT),塔贡组(E1TG)及班塔博组(E1-2BT),其岩石地层特征可与中国滇西兰坪-思茅地区的同时代地层相对比;②在上述11个组级岩石地层单位中均获古生物资料,分属14个生物地层单位,其生物地层特征可与中国滇西兰坪-思茅地区的同时代地层相对比;③万象地区的构造变形可划分为成盐前(晚白垩世)、成盐期(古新世)、成盐后(始新世)3个时期,一级构造为塔贡叠加复式向斜、班普夸快叠加复式背斜;④含盐地层塔贡组(E1TG),为一套乳白、淡红色膏盐层及棕红、紫红色陆源细碎屑岩,膏盐层与陆源细碎屑岩构成3个明显的沉积旋回,据此可划分为3个岩性段、6个岩性层,具工业意义的钾镁盐矿均产于塔贡组下段膏盐层(E1TG1-1)中;⑤塔贡组(E1TG)可划分为滨湖、浅湖、半深湖相,在成盐过程中沉积环境发生过较明显的迁移改组,膏盐层形成于气候持续干旱、盆地基底持续下降、卤水持续补给的沉积环境。  相似文献   

Geochronological and geochemical constraints on the petrogenesis of late Mesoproterozoic mafic and granitic rocks in the southwestern Yangtze Block     

Guichun Liu  Jing Li  Xin Qian  Qinglai Feng  Wei Wang  Guangyan Chen  Shaobin Hu 《地学前缘(英文版)》2021,12(1):39-52

Late Mesoproterozoic igneous rocks in the SW Yangtze Block are important for understanding the role of it in reconstruction of the Rodinia supercontinent.In the present study,we report new geochronological,geochemical,and Nd-Hf isotopic data for the Cuoke plagioclase amphibolites and granites in the SW Yangtze Block.Geochronological results show that the plagioclase amphibolites and granites have similar late Mesoproterozoic zircon U-Pb ages of 1168-1162 Ma,constituting a bimodal igneous assemblage.The plagioclase amphibolites have high and variable TiO2 contents(1.15-4.30 wt.%)and Mg#(34-66)values,similar to the tholeiitic series.They are characterized by enrichment in LREEs and LILEs,and have OIB-like affinities with positive Nb and Ta anomalies.The plagioclase amphibolites have positive whole-rockεNd(t)(+3.2 to+4.3)and zirconεHf(t)(+4.3 to+10.7)values,indicating that they were derived from an OIB-like asthenospheric mantle source.The granites belong to the reduced peralkaline A-type series and have negativeεNd(t)value of-6.0 andεHf(t)values of-5.8 to-13.8,indicating a derivation from the partial melting of ancient mafic lower crust.In combination with the~1.05-1.02 Ga bimodal igneous assemblage in the SW Yangtze Block,we propose that the Cuoke 1168-1162 Ma igneous rocks were likely formed in a continental rift basin and argue against the existance of Grenvillian Orogen in the SW Yangtze Block during the late Mesoproterozoic.  相似文献   

JSL-30型钻机钻进参数检测系统的研究     

赵大军  罗启钟  王君  孙友宏  徐龙宪  于萍  高金梁  计胜利 《地质与勘探》2006,42(3):97-99

钻进参数检测对钻进参数优化、钻机设计、钻进工艺研究具有重要作用.结合JSL-30型钻机结构和工作原理,研制了适用于振动条件下的钻进参数检测系统.经检验,检测数据准确可靠.  相似文献   

Recent Progress of Hemispheric Coupling of Solar Activity Cycle     

ZHANG Xiao-juan  DENG Lin-hua 《Chinese Astronomy and Astrophysics》2021,45(1):1-30

The hemispheric coupling phenomenon of solar activity cycle was discovered as early as the mid-20th century, and it is one of the most common topic in the long-term spatio-temporal evolution of the Sun, while the observational features and physical mechanism of hemispheric coupling have not been completely understood. The theoretical model of solar magnetohydrodynamics driven by this phenomenon is helpful in studying the basic information of the spatio-temporal evolution of solar activity cycle, and is also of great value to the short- and medium-term forecast of solar activity as well as the space weather. Here, we first give the discovery and observational history of the hemispheric coupling of solar activity. And then, the basic observational features of hemispheric coupling at different spatio-temporal scales and their possible mechanism are summarized. Finally, we give a discussion about the important unresolved issues and development trends in this important field.  相似文献   

Research on Pulsar Candidate Identification Method Based on Deep Residual Neural Network     

《Chinese Astronomy and Astrophysics》2021,45(3):364-381

As the next-generation radio astronomical telescopes continuously improve and develop, the pulsar survey will produce millions of pulsar candidates, which pose considerable challenges for pulsar identification and classification. The rapidly evolving artificial intelligence (AI) techniques are being used for pulsar identification and discovery of new pulsars. Using the pulsar data set observed with the Parkes telescope, namely the High Time Resolution Universe Survey (HTRUS), a 14-layer deep residual network has been designed (called the Residual Network, ResNet) for pulsar candidate classifications. In the HTRUS sample data, the number of non-pulsar candidates (i.e., negative samples) is much larger than that of pulsar candidates (i.e., positive samples). The imbalance between the positive and negative samples is prone to result in model misjudgement. By using the over-sampling technique to enhance the data of positive samples in the training set and adjusting the ratio of positive and negative samples, we have solved this imbalance problem. In the training process, the hyperparameters are adjusted by means of 5-fold cross validation to build the model. The test results indicate that the model can achieve a high precision (98%) and recall (100%), the F1-score can reach 99%, and that the implementation of each sample test needs only 7 ms, it has provided a feasible approach for the future big-data analysis of pulsars.  相似文献   

Orbit Determination of the Asteroid (469219) Kamoòalewa and Its Error Analysis     

《Chinese Astronomy and Astrophysics》2021,45(3):402-411

As an Earth co-orbital asteroid, (469219) Kamoòalewa is a near earth object (NEO) with high value of research, and one of the targets explored by the first Chinese asteroid exploration mission. Given its orbit characteristics, we build a refined dynamical model for this asteroid, in which the effects induced by nonspherical gravitational fields of the Sun, the Earth, and the Moon are combined. On the basis of the dynamical model of the asteroid (469219) Kamoòalewa, its orbit is determined with optical data from 2004 to 2018 available on the Minor Planet Center (MPC) database. The root mean square error of post-fit residuals is about 0.2 arc second (comparable with that of the Jet Propulsion Laboratory (JPL)/Horizons), and the post-fit residuals of optical observations in 2004 are decreased. At the end, we implement error analysis on the asteroid (469219) Kamoòalewa's orbit in detail, and also predict its orbit error at the time interval between 2020 and 2025.  相似文献   

The first photometric investigations of the G-type shallow contact binary IO Cnc     

廖文萍  李临甲  周肖  王琪善 《天文和天体物理学研究(英文版)》2021,(2)

IO Cnc was classified to be a new G-type(G0)W UMa-type eclipsing binary system.Our first multicolor photometric solutions show that IO Cnc is a new W-subtype shallow contact binary with a fill-out factor of f=16.1%and a low mass ratio of q=3.12(or 1/q=0.32).During orbital period investigations,a cyclic variation and a downward parabolic variation with a rate of(-1.28±0.43)×10^-7 d yr^-1 was discovered in the observed–calculated(O-C)curve.The cyclic variation was analyzed by the light travel time effect(LTTE)via a potential red dwarf companion star,an orbital semi-major axis shorter than 4.88±0.82 AU was obtained.Finally,we collect physical parameters of a sample of 50 G-type shallow contact binaries(f≤20%),it is suggested that most of the G-type shallow contact binaries are undergoing a longterm and periodic orbital period changes,especially more systems show long-term decreases.The long-term orbital period decrease indicates that IO Cnc is in a mass transferring from the more massive component to the less massive one.With the long-term decrease of the orbital period,this shallow contact binary will evolve into a deeper contact one.  相似文献