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961.
任一特定时期的地质演化都必定源自前期背景,并影响后继地质作用。元古宙的构造特征及晚古生代的地质记录可帮助我们更好地认识早古生代华北板块的构造-沉积演化,这一演化包括4 个阶段。第1 阶段(∈1-∈3)以被动陆缘的发育和全球海平面上升为特点,二者叠加形成强烈的相对海平面上升,并在南、北边缘形成早期沉积。第2 阶段(O1y-O1l)表现为因洋壳俯冲导致的西南部构造抬升及全球海平面下降,二者结合形成的相对海平面下降在华北中部及西南部形成分布广泛的不整合面及白云岩。第3 阶段(O1m-O2)期间,来自南、北的挤压导致以边缘上凸为特点的板块变形,在伴以全球海平面上升的情况下导致轻度的相对海平面上升并形成板块中部局限陆表海的膏岩沉积。第4 阶段(O3-C1)则是强烈的南北挤压和全球海平面下降导致华北大陆板块整体鞍状抬升和长期不整合的发育,该不整合在北部及南部的侵蚀作用明显强于中部。 相似文献
962.
‘Qianzhong Uplift’ and evolution of the Late Paleozoic palaeogeography and its control on formation of bauxite in Guizhou Province
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Deng Xu-Sheng Du Yuan-Sheng Yu Wen-Chao Wu Kai-Bin Lu Shu-Fan Zhang Han-Bin 《古地理学报》1999,22(5):872-892
The Early Paleozoic regional uplift(e.g.,the Qianzhong Uplift)and sea-level changes had obviously controlled the evolution of the Late Paleozoic palaeogeography and paleogeomorphology in Guizhou Province. However,the formation time and evolution of the Qianzhong Uplift is still in debate,which limits the understanding of the Permo-Carboniferous paleogeographic and paleogeomorphologic evolution that formed bauxite in Guizhou. In this paper,based on field surveys and data collection,we established the palaeogeography of several important geological periods from the Late Cambrian to Permian in Guizhou,and re-recognized the formation time and evolution of the Qianzhong Uplift,and revealed the coupling relationship between the Qianzhong Uplift and Guizhou bauxite formation. During the Cambrian to early-middle Early Silurian,the continent-marine transitional facies were missed in the northern margin of the Qianzhong Uplift,central Guizhou Province,such as Bijie,Jinsha and Zunyi. The large-scale uplift of the central Guizhou Province should begin with the tidal flat deposits of the Hanchiatien Formation in the Early Silurian. Because of the Qianzhong Uplift,the central Guizhou and Zunyi areas experienced long-lasting and intense weathering and erosion,forming karst depressions,funnels,and canyons in the Early Carboniferous. The karst landform provided material conditions and location for the formation of bauxite deposits in the Early Carboniferous. The bauxite ore formed under intense chemical wreathing and leaching induced by the glacio-eustasy and paleoclimate fluctuations. The early long-lasting and intense weathering and erosion occurred in the northern Guizhou along with the Permo-Carboniferous glacio-eustasy,had leaded to the formation of coastal wetland and depressions,which were favorable places for the Early Permian bauxite formation. The Early Permian bauxite ores in Guizhou Province have an obvious coupling relationship with the Late Paleozoic Ice Age. 相似文献
963.
本文列举了晚前寒武纪特别是震旦纪动物化石的记录。阐述了地史早期动物演化的主要研究成果及存在的问题,预测在不久的将来该领域定会取得突破性进展。 相似文献
964.
965.
We report the discovery of a variable object in the Hubble Deep Field North (HDF-N) which brightened, during the 8.5 d sampled by the data, by more than 0.9 mag in I 814 and about 0.7 mag in V 606 , remaining stable in B 450 . Subsequent observations of the HDF-N show that two years later this object has dimmed to about its original brightness in I 814 . The colours of this object, its brightness, its time behaviour in the various filters and the evolution of its morphology are consistent with it being a Type Ib supernova in a faint galaxy at z . 相似文献
966.
We present high‐quality spectra of the majority of stars that have been classified as Oe and find that their published spectral types are generally too early, most likely due to infilling of He I lines. As a matter of fact, all stars classified as Oe actually fall inside the range O9–B0 with the important exception of HD 155806 (O7.5 III) and perhaps HD 39680 (difficult to classify, but likely O8.5V). Observations of a sample of objects with published spectral types in the O9–B0 range previously classified as peculiar or emission‐line stars fail to reveal any new Oe star with spectral type earlier than O9.5. Most objects classified as peculiar in “classical” literature show signs of binarity in our spectra, but no spectral anomalies. We conclude that there is likely a real decline in the fraction of Be stars for spectral types earlier than B0, not due to observational bias. The few Oe stars with spectral types earlier than O9.5 deserve detailed investigation in order to provide constraints on the physical reasons of the Be phenomenon. (© 2004 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim) 相似文献
967.
《地震研究进展(英文)》2023,3(1):100197
It is critical to determine whether a site has potential damage in real-time after an earthquake occurs, which is a challenge in earthquake disaster reduction. Here, we propose a real-time Earthquake Potential Damage predictor (EPDor) based on predicting peak ground velocities (PGVs) of sites. The EPDor is composed of three parts: (1) predicting the magnitude of an earthquake and PGVs of triggered stations based on the machine learning prediction models; (2) predicting the PGVs at distant sites based on the empirical ground motion prediction equation; (3) generating the PGV map through predicting the PGV of each grid point based on an interpolation process of weighted average based on the predicted values in (1) and (2). We apply the EPDor to the 2022 MS 6.9 Menyuan earthquake in Qinghai Province, China to predict its potential damage. Within the initial few seconds after the first station is triggered, the EPDor can determine directly whether there is potential damage for some sites to a certain degree. Hence, we infer that the EPDor has potential application for future earthquakes. Meanwhile, it also has potential in Chinese earthquake early warning system. 相似文献
968.
969.
早更新世以来腾格里沙漠形成与演化的风成沉积证据 总被引:3,自引:0,他引:3
对陇西盆地六盘山西侧山麓剥蚀面上厚约223 m的断岘黄土-古土壤剖面的古地磁、磁化率和粒度进行分析,该剖面具有1.8 Ma以来完整的风成沉积旋回。主要应用砂粒百分含量(>63μm)作为指示风成物质来源区沙漠范围和气候干旱的直接指标,初步发现腾格里沙漠自1.8 Ma以来至少有2次大的扩张与变化过程,分别发生在1.1和0.8 MaBP前后,表明腾格里沙漠的扩张与变化可能同全球性的冰量增加和冬季风增强以及区域性的青藏高原隆升有成因上的联系。 相似文献
970.
长江口柱状沉积物中甾醇的组成特征及其地球化学意义 总被引:4,自引:0,他引:4
通过对长江口两个柱状沉积物中有机质的GC-MS分析,检出C27-C29甾烷醇、C27Δ5,C28Δ7和C29Δ22甾烯醇以及C30Δ22烯醇(4α,23,24-三甲基-5α-胆甾-22-烯醇)7种主要甾醇生物标志化合物.8站位沉积物中以陆源输入为主的C29甾醇的相对丰度最高,在17站位深层沉积物中也以C29甾醇为主,而其表层沉积物中则是以海洋浮游动物输入为主的C27甾醇的相对丰度最高.在所有的样品中甾醇都经历了较强的加氢还原作用,相同碳数的甾烷醇的相对丰度远远高于其相对应的甾烯醇的相对丰度.随着沉积深度的增加,甾烯醇的加氢还原作用越强,且由于两个站位不同的沉积环境,8站位甾烯醇的加氢还原作用更强. 相似文献