福田站基坑监控量测信息管理系统的建立与应用     

王昌洪  陈雪丰  王洪战 《测绘信息与工程》2012,37(6):73-75

根据广深港客专福田站超深超宽基坑施工监控量测的需要,应用远程数据通讯技术、数据库技术和GIS技术设计并建立了工程监控量测信息管理管理系统,统计和分析功能提高了监控量测信息的反馈效率,解决了监控量测与施工配合的问题,工程实践表明系统提高了监控量测信息的反馈效率,达到了福田站基坑监控量测信息化管理的需求。  相似文献   

关于超强台风“桑美”强度突变研究的几点思考     

郑峰  吴群 《气象科技》2010,38(5):533-536

超强台风"桑美"在浙江省温州市苍南县登陆,登陆时中心附近最大风力达17级,中心气压920hPa,是近50年来登陆我国大陆最强的台风。为了认识超强台风"桑美"强度突然增强的机制机理,气象工作者做了许多有意义的工作,如"桑美"的观测分析、数值模拟、强度突增原因探究等。文章对以往研究成果进行了简述,指出了目前在此方面研究存在的问题,如数值模拟台风强度突增的量值偏小,强度突增的机理没有新的明显突破,以及气候变暖对台风强度突增如何影响涉及较少等。  相似文献   

Discovery of six high-redshift quasars with the Lijiang 2.4 m telescope and the Multiple Mirror Telescope     

Xue-Bing Wu  Wen-Wen Zuo  Qian Yang  Wei-Min Yi  Chen-Wei Yang  Wen-Juan Liu  Peng Jiang  Xin-Wen Shu  and Hong-Yan Zhou 《天文和天体物理学研究(英文版)》2012,(9):1185-1190

Quasars with redshifts greater than 4 are rare, and can be used to probe the structure and evolution of the early universe. Here we report the discovery of six new quasars with i-band magnitudes brighter than 19.5 and redshifts between 2.4 and 4.6 from spectroscopy with the Yunnan Faint Object Spectrograph and Camera (YFOSC) at the Lijiang 2.4 m telescope in February, 2012. These quasars are in the list of z > 3.6 quasar candidates selected by using our proposed J K/i Y criterion and the photometric redshift estimations from the SDSS optical and UKIDSS near-IR photometric data. Nine candidates were observed by YFOSC, and five among six new quasars were identified as z > 3.6 quasars. One of the other three objects was identified as a star and the other two were unidentified due to the lower signal-to-noise ratio of their spectra. This is the first time that z > 4 quasars have been discovered using a telescope in China. Thanks to the Chinese Telescope Access Program (TAP), the redshift of 4.6 for one of these quasars was confirmed by the Multiple Mirror Telescope (MMT) Red Channel spectroscopy. The continuum and emission line properties of these six quasars, as well as their central black hole masses and Eddington ratios, were obtained.  相似文献   

Periodicity in the most violent solar eruptions： recent observations of coronal mass ejections and flares revisited     

Peng-Xin Gao  Jing-Lan Xie  Hong-Fei Liang 《天体物理学报》2012,(3):322-330

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A numerical study of self-gravitating protoplanetary disks     

Kazem Faghei 《天体物理学报》2012,(3):331-344

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Could bright γ-ray burst optical transients have been recorded historically？     

Richard G. Strom  Fu-Yuan Zhao  Cheng-Min Zhang 《天体物理学报》2012,(3):260-268

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Reanalysis of the RXTE observations of the black-hole candidate XTE J1650–500 in the 2001/2002 outburst     

Li-Hong Yan  Jian-Cheng Wang 《天体物理学报》2012,(3):269-286

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Two-dimensional Numerical Modeling Research on Continent Subduction Dynamics   总被引：3，自引：0，他引：3  

WANG Zhimin  XU Bei  ZHOU Yaoqi  XU Hehua  HUANG Shaoying The Key Laboratory of Orogenic Belts  Crustal Evolution 《《地质学报》英文版》2004,78(1):313-319

Continent subduction is one of the hot research problems in geoscience. New models presented here have been set up and two-dimensional numerical modeling research on the possibility of continental subduction has been made with the finite element software, ANSYS, based on documentary evidence and reasonable assumptions that the subduction of oceanic crust has occurred, the subduction of continental crust can take place and the process can be simplified to a discontinuous plane strain theory model. The modeling results show that it is completely possible for continental crust to be subducted to a depth of 120 km under certain circumstances and conditions. At the same time, the simulations of continental subduction under a single dynamical factor have also been made, including the pull force of the subducted oceanic lithosphere, the drag force connected with mantle convection and the push force of the mid-ocean ridge. These experiments show that the drag force connected with mantle convection is critical fo  相似文献   

中天山、伊犁及塔里木地块开始参与Rodinia超大陆聚合过程早于新元古代?   总被引：2，自引：0，他引：2  

蔡志慧  马绪宣  何碧竹 《地质学报》2019,93(10):2426-2445

长久以来,中国主要陆块被普遍认为比世界其他陆块开始参与罗迪尼亚超大陆聚合的时间较晚,为新元古代早期。为了探讨此问题,我们选择中国中天山、伊犁及塔里木地块作为主要研究对象,系统分析了新元古代早期(1.0～0.8Ga)的构造变形及岩浆特征。新元古代早期构造变形主要表现为拉伸线理近平行于造山带方向,反映了后造山陆内走滑剪切过程。1.0～0.8Ga的岩浆岩皆为较小规模花岗岩,未见基性包体,矿物组合中基本无角闪石,具有高钾钙碱性和过铝质特征,并含有大量捕获老锆石,说明古老基底或重熔地壳的显著参与。岩石源区主要为重熔基性下地壳,在构造背景判别图上基本落在后造山环境。锆石Ti及全岩Zr温度计算结果显示这些岩体的结晶温度普遍偏高,约800℃。结合已有区域地质资料,我们认为:①在新元古代原塔里木陆块(包括早期中天山、伊犁及塔里木地块)已经位于罗迪尼亚超大陆内部,1.0～0.8Ga变形及岩浆记录皆反映了原塔里木陆块与其它陆块碰撞后的构造事件;②由于超大陆聚合后的热毯效应使得新元古代早期花岗岩结晶温度偏高;③中天山、伊犁及现今塔里木地块最初参与罗迪尼亚超大陆汇聚的时间应早于新元古代(1.0Ga)。  相似文献   

西昆仑北缘主乌鲁克锰矿床地质特征及成因探讨          下载免费PDF全文

毛红伟 《地质找矿论丛》2019,34(1):72-77

主乌鲁克锰矿床位于西昆仑北缘晚古生代陆缘裂谷恰尔隆弧盆系的北部,含锰层位为下石炭统他龙群细碎屑岩夹碳酸盐岩,锰矿层为黑色泥质碳质页岩夹铁锰质泥晶灰岩。锰矿体严格受地层的控制,呈NWW向展布,延伸较为稳定,规模较大,共见有13条锰矿体,其中有3个矿体较大构成主矿体;锰矿石以原生菱锰矿为主体,氧化矿石不多。该矿床与近年发现的玛尔坎苏地区锰矿床既有相似之处,又有明显不同,矿床类型为在深海-半深海陆缘裂谷环境中形成的与黑色碳质页岩有关的沉积型锰矿床,锰矿的成矿时代为早石炭世。由于下石炭统他龙群是西昆仑地区新发现的含锰层位,具有较大的找矿潜力,应加强矿床外围及深部的找矿工作。  相似文献