物质点强度折减法边坡失稳判据选择方法     

蒋先平  张鹏  卢艺伟  刘磊磊  张明辉 《地质科技情报》2022,41(2):113-122

用物质点强度折减法求解边坡安全系数时,需要选择一定的失稳判据,而采用不同的失稳判据获得的安全系数通常存在一定差异.为此,采用物质点强度折减法对两个边坡算例进行了稳定性分析,对比研究了文献中常用的4种边坡失稳判据(计算不收敛、特征点位移突变、塑性应变贯通及界限值判据)在计算边坡安全系数时的合理性及适用性.同时,将Spen...  相似文献   

XUV Photometer System (XPS): Improved Solar Irradiance Algorithm Using CHIANTI Spectral Models     

Thomas N. Woods  Phillip C. Chamberlin  W. K. Peterson  R. R. Meier  Phil G. Richards  Douglas J. Strickland  Gang Lu  Liying Qian  Stanley C. Solomon  B. A. Iijima  A. J. Mannucci  B. T. Tsurutani 《Solar physics》2008,250(2):235-267

Solar soft X-ray (XUV) radiation is highly variable on all time scales and strongly affects Earth’s ionosphere and upper atmosphere; consequently, the solar XUV irradiance is important for atmospheric studies and for space weather applications. Although there have been several recent measurements of the solar XUV irradiance, detailed understanding of the solar XUV irradiance, especially its variability during flares, has been hampered by the broad bands measured in the XUV range. In particular, the simple conversion of the XUV photometer signal into irradiance, in which a static solar spectrum is assumed, overestimates the flare variations by more than a factor of two as compared to the atmospheric response to the flares. To address this deficiency in the simple conversion, an improved algorithm using CHIANTI spectral models has been developed to process the XUV Photometer System (XPS) measurements with its broadband photometers. Model spectra representative of quiet Sun, active region, and flares are combined to match the signals from the XPS and produce spectra from 0.1 to 40 nm in 0.1-nm intervals for the XPS Level 4 data product. The two XPS instruments are aboard NASA’s Solar Radiation and Climate Experiment (SORCE) and Thermosphere, Ionosphere, Mesosphere, Energetics, and Dynamics (TIMED) satellites. In addition, the XPS responsivities have been updated for the latest XPS data processing version. The new XPS results are consistent with daily variations from the previous simple conversion technique used for XPS and are also consistent with spectral measurements made at wavelengths longer than 27 nm. Most importantly, the XPS flare variations are reduced by factors of 2 – 4 at wavelengths shorter than 14 nm and are more consistent, for the first time, with atmospheric response to solar flares. Along with the details of the new XPS algorithm, several comparisons to dayglow and photoelectron measurements and model results are also presented to help verify the accuracy of the new XUV irradiance spectra.  相似文献   

High Spatial Resolution X-Ray Spectroscopy of Cas A with Chandra     

Xue-Juan Yang Fang-Jun Lu Li Chen 《中国天文和天体物理学报》2008,8(4)

We present high spatial resolution X-ray spectroscopy of the supernova remnant Cassiopeia A with the Chandra observations. The X-ray emitting region of this remnant was divided into 38 × 34 pixels of 10″× 10″ each. Spectra of 960 pixels were created and fitted with an absorbed two component non-equilibrium ionization model. From the results of the spectral analysis we obtained maps of absorbing column density, temperatures, ionization ages, and the abundances of Ne, Mg, Si, S, Ca and Fe. The Si, S and possibly Ca abundance maps show obvious jet structures, while Fe does not follow the jet but seems to be distributed perpendicular to it. The abundances of Si, S and Ca show tight correlations between one another over a range of about two dex. This suggests that they are ejecta from explosive Oburning and incomplete Si-buming. Meanwhile, the Ne abundance is well correlated with that of Mg, indicating them to be the ashes of explosive C/Ne burning. The Fe abundance is positively correlated with that of Si when the latter is lower than 3 times the solar value, and is negatively correlated when higher. We suggest that such a two phase correlation is due to the different ways in which Fe was synthesized.  相似文献   

A GRB Follow-up System at the Xinglong Observatory and Detection of the High-Redshift GRB 060927     

Wei-Kang Zheng Jin-Song Deng Meng Zhai Li-Ping Xin Yu-Lei Qiu Jing Wang Xiao-Meng Lu Jian-Yan Wei Jing-Yao Hu 《中国天文和天体物理学报》2008,8(6)

A gamma-ray burst (GRB) optical photometric follow-up system at the Xinglong Observatory of National Astronomical Observatories of China (NAOC) has been constructed. It uses the 0.8-m Tsinghua-NAOC Telescope (TNT) and the 1-m EST telescope, and can au-tomatically respond to GRB Coordinates Network (GCN) alerts. Both telescopes slew rela-tively fast, being able to point to a new target field within ～ 1 min upon a request. Whenever available, the 2.16-m NAOC telescope is also used. In 2006 the system responded to 15 GRBs and detected seven early afterglows. In 2007 six GRBs have been detected among 18 follow-up observations. TNT observations of the second most distant GRB 060927 (z = 5.5) are shown, which started as early as 91 s after the GRB trigger. The afterglow was detected in the combined image of the first 19 × 20 s unfiltered exposures. This GRB follow-up system has joined the East-Asia GRB Follow-up Observation Network (EAFON).  相似文献   

水资源全成本定价问题   总被引：2，自引：1，他引：1  

俞路  姚天祥 《地域研究与开发》2004,23(1):69-72

随着经济的发展,人们对水资源的需求越来越多,水资源的天然供给与人类需求的矛盾越来越突出。在我国一些地区水资源不足已成为制约经济发展的一个主要瓶颈。但是一方面是水资源的不足,一方面又存在水资源的大量浪费,因此,合理配置水资源的使用已成为当务之急。配置资源的方式有2种,一种是计划手段,一种是经济手段,水资源的合理配置应将2种方法结合使用。文章依据马克思的劳动价值论,对水资源全成本定价方法进行了探讨。  相似文献   

Disaster risk evaluation using factor analysis: a case study of Chinese regions     

Chen  Ning  Chen  Lu  Tang  Chaosheng  Wu  Zhengjiang  Chen  An 《Natural Hazards》2019,99(1):321-335

Natural Hazards - Regional risk to natural disasters is a critical multi-criteria decision-making (MCDM) problem in the literature due to the complicated and usually conflicting evaluation index...  相似文献   

中蒙俄毗邻地区中蒙古—额尔古纳成矿带成矿地质条件与成矿特征     

柴璐  李霄  周永恒 《地质论评》2019,65(Z1):257-258

正介于蒙古—鄂霍次克断裂带和中蒙古—得尔布干断裂带之间的中蒙古—额尔古纳成矿带,西起蒙古杭爱山,经中戈壁省、乔巴山,向东延伸至我国大兴安岭北段满洲里—呼吗一带,封闭于俄罗斯阿穆尔州,中国境内部分包括了大兴安岭成矿省的上黑龙江(边缘海)Au(Cu-Mo)成矿带和额尔古纳Cu-Mo-Pb-Zn-Ag-Au—萤石成矿亚带(徐志刚等,2008;朱群等,2014)。  相似文献   

粤东塘唇石英脉型钨(锡)矿床地质特征、成矿时代及其找矿意义          下载免费PDF全文

卢友月  付建明  张国培  郑宗皓  李楠  程顺波  秦拯纬  马丽艳 《地球科学》2019,44(2):387-398

塘唇钨(锡)矿是近年来新发现的一个具有大型规模找矿潜力的石英脉型矿床.矿床产于粤东龙窝花岗闪长岩岩体西部外接触带,赋矿地层为下侏罗统金鸡组碎屑岩,该层位是南岭及邻区石英脉型钨锡矿的最新赋矿地层.在详细的野外地质调查基础上,对矿床含钨石英脉中的白云母进行⁴⁰Ar-³⁹Ar测年,获得白云母⁴⁰Ar-³⁹Ar坪年龄为150±1 Ma,等时线年龄为149±2 Ma(MSWD=1.20),它们在误差范围内一致,为南岭地区燕山早期大规模成岩成矿作用高峰期的产物.塘唇钨(锡)矿的发现,不仅拓宽了石英脉型钨锡矿的找矿视野,还有助于完善石英脉型钨锡矿成矿规律和成矿模式,对区域下一步找矿具有重要指导意义.  相似文献   

塔里木盆地塔中北坡奥陶系微生物碳酸盐岩储层形成机制与评价          下载免费PDF全文

王玉伟  陈红汉  曹自成  云露 《地球科学》2019,44(2):559-571

微生物岩储层是当前的研究热点之一.通过对塔中北坡微生物岩样品的岩芯以及铸体薄片的观察,发现研究区域的微生物岩储层以裂缝-孔隙型储层为主.对其进行全直径孔渗性检测发现,微生物岩储层具有较好的天然气储集物性.通过对微生物岩的形成机制及特点的分析,结合应力敏感实验和成像测井资料,总结出微生物岩储集空间发育的优势因素.原生白云石的生成可以促进方解石的溶解,而塔中北坡微生物岩发生早成岩岩溶作用,部分地区叠加晚期深成热液改造,提高了储集物性;有机质含量较丰富不仅可以在埋藏成岩阶段生成有机酸造成溶蚀,还能够降低微生物岩的极限强度从而容易在构造作用下发生断裂形成裂缝,因此塔中北坡微生物岩储集空间主要以次生作用为主.通过岩石压缩系数的测定,得出微生物岩的抗压实能力一般,但藻屑骨架对藻孔的保护有利,抗压实能力最强的是受到热液作用而硅化的微生物岩,其次是白云石化微生物岩.  相似文献   

利用深地震反射剖面开展矿集区深部结构的探测:现状与实例          下载免费PDF全文

刘子龙  卢占武  贾君莲  李文辉  任彦宗 《地球科学》2019,44(6):2084-2105

深地震反射剖面技术以其探测精度高的优势被作为岩石圈精细结构研究的先锋技术,并在全球典型矿集区结构探测中发挥了重要作用.为深入研究青藏高原碰撞造山成矿系统深部结构与成矿过程,本文系统总结了深地震反射技术发展现状,梳理了该技术在加拿大、澳大利亚、中国、俄罗斯、瑞典等全球多个国家的典型矿集区的应用实例,归纳总结了地壳深部结构对矿集区控矿因素的影响,阐述了地壳、上地幔深部结构与深部成矿过程的关系.从全球实例看,深地震反射剖面探测成果为大型矿集区的形成提供了深部线索,反射透明区可能是地幔流体向上运移通道,形成矿集区的成矿物质与能量来源,表明地幔物质参与了成矿作用;具有很强反射特征的断裂系统,包括大型断层、滑脱面和剪切带,是成矿流体从下地壳向上迁移的通道;矿集区深地震反射剖面中“亮点”反射可能是火山活动的深部岩浆上涌至中地壳后而形成的残余岩浆囊的反映.揭露精细的矿集区深部结构不但对矿集区构造历史演化的重建具有重要作用,还对未来成矿潜力和前景靶区的确定具有重要指导意义.  相似文献