Sedimentary records of the late Early Cretaceous compressional setting in the South China block: A case study of the Xingning Basin,Guangdong Province     

Jintao Kong  Zhongjie Xu  Yunyi Liang  Rihui Cheng 《Island Arc》2021,30(1):e12399

Recently, some scholars have proposed that the South China Block (SCB) was controlled by a compressive tectonic regime in the middle–late Early Cretaceous, challenging the belief that the SCB was under an extensional setting during the Cretaceous. The Early Cretaceous tectonic setting constraint in the SCB can offer vital insight to clarify the Mesozoic subduction history of the Paleo-Pacific. Therefore, to determine the SCB tectonic regime during the Early Cretaceous, this study investigated sedimentary rocks from the Lower Cretaceous Heshui Formation in the Xingning Basin, a foreland basin located in the southeastern SCB. Provenance analysis was performed using sandstone modal analysis, sandstone geochemical characteristics, and detrital zircon geochronology. Based on the results, we discussed basin sediment sources and the SCB tectonic regime during the Early Cretaceous. The results showed that the maximum Heshui Formation depositional age was 103 Ma ± 1.6 Ma in the Early Cretaceous Albian. Detrital framework modes and geochemical characteristics of sandstone indicated that Heshui Formation's source rocks were granites and sedimentary rocks. The detrital zircon U–Pb ages could be classified into two major and four subordinate age populations. The Wuyi Terrane to the north and southeast coastal regions to the east were the primary potential Heshui Formation source areas. However, the lower and upper sandstones are different in the peak ages, ~437 and ~146 to 104 Ma, respectively, indicating that the major source area shifted from the Wuyi Terrane to the southeastern coastal regions during the late Early Cretaceous. The sandstone modal analysis results indicated that the source area comprised mainly collisional–orogenic material. The SCB was under a compressive tectonic regime during the late Early Cretaceous and this compression action continued until at least 103 Ma ± 1.6 Ma.  相似文献   

A Study of the Scale Height of the Thin Galactic Disk in the Solar Neighborhood     

Da-Li Kong  Zi Zhu 《Chinese Astronomy and Astrophysics》2008

An attempt is made to determine the scale height of the thin Galactic disk in the solar neighborhood using various stellar samples from the accurate astrometric data of the Hipparcos satellite. Using the Tycho color indices and considering the completeness of the samples, several samples were selected from the main sequence and the horizontal branch. Based on two rather complete samples, it is found that the scale height of the Galactic disk defined by the O-B type main sequence stars is 103.1 ± 3.0 pc and the Sun is located at height of 15.2 ± 7.3 pc above its mean plane; while the scale height of the Galactic disk defined by the horizontal branch stars is 144.0 the ±10.0 pc and the Sun is located at height 3.5 ± 5.4 pc above the mean plane. Owing to the incompleteness of observational samples, it is not possible to use the main sequence stars of spectral types A, F, G, K and M to make a reliable determination of the scale height.  相似文献   

Observations of Giant Pulses of the Crab Pulsar     

Ling-Jun Kong  Ali Esamdin  Cheng-Shi Zhao  Zhi-Yong Liu  Jian-Ping Yuan 《中国天文和天体物理学报》2008,8(3):277-284

The Crab Pulsar was observed at 1540 MHz with the 25m radio telescope at Urumqi with a filterbank de-dispersion backend. A total of 2436 giant pulses with pulse energies larger than 4300 Jy μs were detected in two observing sets. All of these giant pulses are located in the main pulse (MP) and inter pulse (IP) windows of the average profile of the Crab Pulsar. The ratio of the numbers of giant pulses detected in the IP and MP windows is about 0.05. Our results show that, at 1540 MHz, the emission in the IP is contributed by giant and normal pulses, while that in the MP is almost dominated by giant pulses. The distribution of energy of the 2436 giant pulses at 1540 MHz can be described by a power-law with index α=3.13±0.09. The intrinsic threshold of giant pulse energy in the MP window is about 1400 Jy μs at 1540 MHz.  相似文献   

Oxygen and Carbon Isotopes of Cold-water Corals—Reconstructing Paleotemperature Changes and Calcification Mechanism     

Le Kong  Enqing Huang  Jun Tian 《地球科学进展》2019,34(12):1252-1261

Cold-water corals represent an intriguing paleoceanographic archive with a great potential to reconstruct high-resolution paleoenvironmental changes. Compared to those of shallow-water corals, proxies derived from cold-water corals have been complicated by biologically mediated vital effects. The oxygen and carbon stable isotope compositions of cold-water coral skeletons are more depleted than the expected carbonate-seawater equilibrium values by 4‰~6‰ and about 10‰, respectively. Therefore, it is necessary to correct for the vital effects before using δ¹⁸O as a temperature proxy. The principles and methods of reconstructing paleotemperature variations of intermediate and deep oceans using oxygen and carbon isotopes of cold-water corals are reviewed, as well as three existing cold-water coral calcification models and their advantages and disadvantages. It is suggested that further micro-scales analysis and targeted experiments are required to clarify the calcification processes of cold-water corals.  相似文献   

山东黄县盆地古近系李家崖组含煤岩系沉积相特征及演化          下载免费PDF全文

孔凡飞  贾强  李增学  吕大炜  刘海燕  王东东  韩乔羽 《古地理学报》2019,21(3):469-478

山东黄县盆地是中国东部一个重要的煤和油页岩共生盆地,古近系李家崖组是盆地主要的含煤岩系发育层段。根据层序地层学理论,建立了古近系层序地层格架;依据钻测井、岩心资料划分了李家崖组的沉积相类型,编制了分体系域的沉积相图。主要结论如下:(1)李家崖组发育湖泊、辫状河三角洲以及扇三角洲3种沉积相类型。(2)层序Ⅰ低水位体系域以辫状河三角洲相为主,湖扩展体系域以扇三角洲相和湖泊相为主,高水位体系域以扇三角洲相为主;层序Ⅱ低水位体系域以辫状河三角洲相为主,湖扩展体系域以扇三角洲相和湖泊相为主,高水位体系域以湖泊相为主。(3)层序Ⅰ发育时期: 低水位期盆地初始形成—湖扩展期盆地扩张—高水位期盆地萎缩;层序Ⅱ发育时期: 低水位期盆地再次缓慢扩张—湖扩展期盆地加速扩张—高水位期盆地萎缩消亡。  相似文献   

Ultimate bearing capacity of energy piles in dry and saturated sand     

Liu  Han-long  Wang  Cheng-long  Kong  Gang-qiang  Bouazza  Abdelmalek 《Acta Geotechnica》2019,14(3):869-879

Acta Geotechnica - The influence of thermal loads on the ultimate bearing capacity of energy piles is examined. Five laboratory model tests were carried out to investigate piles equipped with...  相似文献   

地面臭氧的变化规律和计算方法的初步研究Ⅱ.可见光波段   总被引：7，自引：0，他引：7  

白建辉  王庚辰  陈辉  徐永福  石立庆  黄忠良  孔国辉  孟泽 《气候与环境研究》2002,7(3):311-320

通过对广州鼎湖山近地面O3、NOx、太阳辐射,气象参数等项目的观测和理论分析,研究了地面O3与NOx等微量气体及太阳可见光辐射的变化规律,详细讨论了可见光波段、不同天气条件地面O3与NOx、光化学反应、气溶胶、可见光辐射等之间复杂的关系.提出以光能量传输与守恒的观点来考虑大气中与可见光辐射有关的主要过程,并以此来研究大气光化学过程中所遵循的能量规律,建立了一个简单、实用、省时的统计模式,用于计算地面O3浓度.结果表明:不同情况下,计算值与观测值吻合得均比较一致.  相似文献   

A model of Saturn inferred from its measured gravitational field     

Dali Kong  Keke Zhang  Gerald Schubert  John D.Anderson 《天文和天体物理学研究(英文版)》2018,(4)

We present an interior model of Saturn with an ice-rock core,a metallic region,an outer molecular envelope and a thin transition layer between the metallic and molecular regions.The shape of Saturn’s 1 bar surface is irregular and determined fully self-consistently by the required equilibrium condition.While the ice-rock core is assumed to have a uniform density,three different equations of state are adopted for the metallic,molecular and transition regions.The Saturnian model is constrained by its known mass,its known equatorial and polar radii,and its known zonal gravitational coefficients,J_(2n),n=1,2,3.The model produces an ice-rock core with equatorial radius 0.203 R_S,where R_S is the equatorial radius of Saturn at the 1-bar pressure surface;the core densityρ_c=10388.1 kgm~(3)corresponding to 13.06 Earth masses;and an analytical expression describing the Saturnian irregular shape of the 1-bar pressure level.The model also predicts the values of the higher-order gravitational coefficients,J_8,J_10 and J_12,for the hydrostatic Saturn and suggests that Saturn’s convective dynamo operates in the metallic region approximately defined by 0.2 R_Sre0.7 R_S,where r_e denotes the equatorial radial distance from the Saturnian center of figure.  相似文献   

青藏铁路沿线不同类型挡沙墙阻沙率     

杨印海  薛春晓  石龙  李凯崇  孔令伟  张芳 《中国沙漠》2020,40(1):173-178

基于风洞试验对青藏铁路沿线不同类型防沙措施防沙效果进行模拟研究，探讨了不同类型挡沙墙的防沙效果。结果表明：挂板式、轨枕式和箱式挡沙墙输沙率随高度基本呈递增缓变型趋势，最大输沙率低于20%；铃铛式和高立式聚乙烯（PE）网挡沙墙随高度呈递减陡降型趋势，距地表6~8 cm处为转折点，转折点以上输沙率随高度增大急剧减小，转折点以下输沙率随高度变化较为平缓，最大输沙率低于50%。随着风速的增大，各挡沙墙的阻沙率呈递减趋势：挂板式和轨枕式挡沙墙对风速的敏感性最弱，整体阻沙效果较优，可大范围推广；箱式挡沙墙对风速的敏感性较弱，建议在风速18 m·s^-1以下的地区使用；PE网挡沙墙防沙效果对风速的敏感性最强，建议在风速10 m·s^-1以下的地区使用。  相似文献   

基于时间序列遥感数据的嵯岗国家沙化土地封禁保护成效评估     

田海静  孙涛  刘旭升  孔祥吉 《中国沙漠》2019,39(3):155-162

2013年中国启动实施了内蒙古自治区新巴尔虎左旗嵯岗国家沙化土地封禁保护区试点。本研究利用2001—2017年生长季NDVI数据分析了嵯岗封禁保护区及周边区域植被长势时空演变特征，分析了多年的生长季降水量和历年旱情，之后利用植被降水利用效率和NDVI残差趋势分析对保护成效进行了评估。结果表明：（1）封禁项目实施之前，封禁区内外植被长势变化趋势基本一致，而在项目实施后的2016、2017年，封禁区内NDVI距平明显高于封禁区外；（2）降水为影响该区域植被长势的主导气候因素，在封禁实施后的2015—2017年该区域连续3 a干旱，极大地限制了区域植被生长；（3）封禁区内植被降水利用效率和NDVI残差均呈现明显的增加趋势，而封禁区外变化不明显，说明封禁提升了植被的自我修复能力；（4）嵯岗封禁保护区由3个地块组成，其中嵯岗林场封禁效果比牧场八队和牧场十一队明显。国家沙化土地封禁保护措施有效促进了植被自我修复，提高了沙漠生态系统应对气候变化的能力。  相似文献