汉江上游晏家棚段全新世古洪水研究     

吉琳  庞奖励  黄春长  查小春  周亚利  刘涛  王蕾彬 《地球科学进展》2015,30(4):487-494

通过对汉江上游详尽的野外考察,在湖北郧县晏家棚河段全新世黄土—古土壤地层中发现3层典型古洪水滞流沉积物。在沉积学的基础上,使用OSL技术断代,确定3期特大洪水事件分别在1 000~900 a BP,1 800~1 600 a BP和3 200~2 800 a BP期间发生。采用"古洪水SWD尖灭点高程法"确定这3期古洪水事件的洪峰水位介于176.20~176.73 m。运用Arc GIS耦合HEC-RAS水力模型,推求这3期古洪水事件的洪峰流量介于53 770~55 950 m3/s,并从多种角度验证了该模型计算结果的科学性和合理性。将此结果与实测洪水和历史洪水资料接续,构成万年尺度洪水水文数据序列,得到汉江上游晏家棚河段万年一遇和千年一遇洪水的流量分别为59 100和45 200m3/s。采用HEC-RAS模型对研究河段进行古洪水模拟,方法科学,结果可靠。将该河段洪水水文数据序列有效地延长到万年尺度,极大地提高了设计洪水的可靠性。  相似文献   

花岗岩的成岩时代、地球化学特征和成因青海祁漫塔格地区虎头崖矿床Ⅵ矿带     

姚磊  吕志成  于晓飞  庞振山  蔡煜琦  刘鹏  刘长城  王凤兰 《吉林大学学报(地球科学版)》2015,(3)

利用 LA ICP MS 锆石 U Pb 法,测得与成矿有关的青海祁漫塔格地区虎头崖矿床Ⅵ矿带花岗岩的成岩年龄为(233.6±1.8)Ma(MSWD=1.2,n=17)。地球化学特征显示：花岗岩属高钾钙碱性、弱过铝质花岗岩;样品的稀土元素组成以总体右倾,轻、重稀土分异明显和具明显的负铕异常为特征;微量元素具有富集 Rb、Th、U、La、Nd 等大离子亲石元素,亏损 Ba、Sr、Nb、P、Ti 等元素的特点。Sr Nd 同位素组成特征显示,花岗岩的源区可能是富集岩石圈地幔。初步研究认为,虎头崖矿床Ⅵ矿带花岗岩可能形成于中、晚三叠世碰撞后碰撞的构造背景下。  相似文献   

Sedimentary and hydrological studies of the Holocene palaeofloods in the Shanxi-Shaanxi Gorge of the middle Yellow River,China     

Xiaogang Li  Chun Chang Huang  Jiangli Pang  Xiaochun Zha  Yugai Ma 《International Journal of Earth Sciences》2015,104(1):277-288

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河北省重污染天气分型及其预报概念模型研究     

王琼  沈瑞珊  庞杨 《气象与环境科学》2020,43(4):107-114

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EFFECTIVE TEMPERATURE COMFORT INDICES FOR SOME MALAYSIAN TOWNS     

Mohammed Ilyas  MSc.  Ph.D.    Pang Chong Yen  BSc.  Chan Ah Wah  BSc. 《Singapore journal of tropical geography》1981,2(1):27-31

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The Moho depth in the Canadian Basin and its tectonic implications          下载免费PDF全文

Ma Yuanyuan  Zhao Lihong  Ling Zilong  Yang Mingming  Pang Beibei 《极地研究》1988,31(3):284

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中国建设用地变化的空间分异特征   总被引：2，自引：0，他引：2  

王文刚  庞笑笑  宋玉祥  李汝资 《地域研究与开发》2012,31(1):110-115

采用变异系数、希尔指数与空间自相关方法对我国2002—2008年建设用地变化的区域差异及空间相关性进行了探讨。结果显示:(1)2002—2008年我国区域建设用地的变化差异总体上呈减小趋势,但区域差异仍较为明显。(2)我国区域建设用地的增长呈现明显的空间二元结构,东部地区"高高"聚集,西部地区"低低"聚集。当前我国土地利用处于"倒U"型变化曲线的顶部区域,土地利用的压力依然很大,应根据土地利用变化的差异性及空间相关性,科学地制定区域土地供给政策。  相似文献   

Holocene environmental change inferred from the loess–palaeosol sequences adjacent to the floodplain of the Yellow River, China     

Chun Chang Huang  Jiangli Pang  Hongxia Su  Shengli Li  Benwei Ge 《Quaternary Science Reviews》2009,28(25-26):2633-2646

Chinese loess deposits are generally considered to be the product of dust storms and dust falls from the central Asia arid zones that were transported across China by the northwesterly continental monsoon. In contrast, the Zhengzhou Loess found southeast of the Loess Plateau, adjacent to the floodplain of the Yellow River, records a different eolian regime and dust source. The Zhengzhou Loess was investigated by field observations, measurements of magnetic susceptibility, particle-size distribution, loss-on-ignition, CaCO₃ and chemical contents. Both field observations and the laboratory results indicate that, during the last glacial, the Zhengzhou Loess was supplied by two different eolian regimes and dust sources, one was from the fresh flood deposits of the Yellow River driven by the northeast winds from the low-lying floodplain, and the other was from the dust storms and dust falls that traveled across the Loess Plateau driven by the northwesterly continental monsoon from the central Asian arid lands. The early Holocene, 11,500–8500 a BP, was a transition during the change in eolian regime and dust source because of the weakened northwesterly monsoon along with the global climatic amelioration. Following the retreat of the northwesterly monsoon from the onset of the mid-Holocene Climatic Optimum at 8500 a BP, dust supply from the drifting sand zone on the Yellow River floodplain became dominant because of the intensified strength of the northeast winds from the Bohai Sea. From 3100 a BP onwards, climatic aridity and extensive human disturbance have resulted in intensive eolian processes causing the incursion of the drifting sand into the Zhengzhou Loess zone. These results show that loess accumulation is more complex than traditionally assumed. The origin of loess deposits elsewhere outside the Loess Plateau may be related to dust sources derived from alluvial sediments of major river systems.  相似文献   

Origin of crude oils with unusually high dibenzothiophene concentrations in the Tazhong Uplift,Tarim Basin     

Sumei Li  Maowen Li  Xiongqi Pang  Haijun Yang  Qiaoyuan Gu 《Journal of Geochemical Exploration》2009

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Star formation in the starburst cluster in NGC 3603     

Matteo Correnti  Francesco Paresce  Rossella Aversa  Giacomo Beccari  Guido De Marchi  Marcella Di Criscienzo  Xiaoying Pang  Loredana Spezzi  Elena Valenti  Paolo Ventura 《Astrophysics and Space Science》2012,340(2):263-279

We have used new, deep, visible and near infrared observations of the compact starburst cluster in the giant HII region NGC 3603 and its surroundings with the WFC3 on HST and HAWK-I on the VLT to study in detail the physical properties of its intermediate mass (∼1–3 M_⊙) stellar population. We show that after correction for differential extinction and actively accreting stars, and the study of field star contamination, strong evidence remains for a continuous spread in the ages of pre-main sequence stars in the range ∼2 to ∼30 Myr within the temporal resolution available. Existing differences among presently available theoretical models account for the largest possible variation in shape of the measured age histograms within these limits. We also find that this isochronal age spread in the near infrared and visible Colour-Magnitude Diagrams cannot be reproduced by any other presently known source of astrophysical or instrumental scatter that could mimic the luminosity spread seen in our observations except, possibly, episodic accretion. The measured age spread and the stellar spatial distribution in the cluster are consistent with the hypothesis that star formation started at least 20–30 Myrs ago progressing slowly but continuously up to at least a few million years ago. All the stars in the considered mass range are distributed in a flattened oblate spheroidal pattern with the major axis oriented in an approximate South-East–North-West direction, and with the length of the equatorial axis decreasing with increasing age. This asymmetry is most likely due to the fact that star formation occurred along a filament of gas and dust in the natal molecular cloud oriented locally in this direction.  相似文献