地震站网全流程一体化监控平台建设进展     

王坦  师宏波  韩宇飞  代光辉  黄经国  刘艳琼  杨陈  祝杰  姬运达 《地震地磁观测与研究》2020,41(4):270-274

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浅析四川省金矿床资源储量概况及成矿类型     

宋元宝  杨怀超  白富政  张伟  牟昀屹  侯从强  杨志军  王丹 《四川地质学报》2020,40(1):56-59,63

四川省岩金矿主要分布于阿坝州北部-东部及甘孜州和凉山州-盆地西部地区,其次是广元市-绵阳市西北部的"金三角"地区的分布特征。通过研究和归纳,本文将矿床类型归纳为11个三级亚类,并根据该11个类型对矿床规模进行统计,得出了数量上四川省以岩浆热液型金矿为主,其次为砂矿性金矿为主,再次为海相火山岩型金矿的结论。在此基础上,对四川省的金矿勘查工作程度、开发利用情况进行了评述,希望能够起到抛砖引玉作用,为省内金矿的勘查开发利用及找矿提供一定思路。  相似文献   

中国北方岩溶地下水污染分析   总被引：5，自引：0，他引：5  

高旭波  王万洲  侯保俊  高列波  张建友  张松涛  李成城  姜春芳 《中国岩溶》2020,39(3):287-298

近年来，受气候变化和强烈人类活动的影响，环境物质及能量多频次、大范围的输入，极大程度上改变着岩溶水系统的水环境质量，岩溶水生态环境遭受不同程度的威胁和破坏，岩溶水水质日趋恶化。本文归纳分析了我国北方岩溶水系统水质特征、污染现状、污染来源及污染途径。我国北方岩溶水水质类型中硫酸盐型水和氯化物型水的分布逐渐增加，主要污染组分为总硬度、SO42-、F-、NO3-和TDS等。其中硫酸盐和硝酸盐污染强度和范围最大，呈现出显著的人类活动影响特征。依据我国北方岩溶系统结构及水力学特征，将岩溶水污染途径概括为:①连续入渗型——主要包括岩溶区地表水（河流、水库等）渗漏污染，城镇污水渠或排污管道破损引起的污水渗漏污染；②越流型污染——污染孔/裂隙水（含矿坑水/老窑积水等）越流污染岩溶水；③间歇入渗型——固废淋溶入渗和污水灌溉渗漏污染等。据此提出了推进岩溶水水资源保护和污染防治的合理化建议。   相似文献   

基于纵横波保幅分离的粘弹介质弹性波正演模拟     

侯志强  尹文笋  李键  孙永壮  刘云 《中国海洋大学学报(自然科学版)》2020,(1):82-92

地下介质往往表现为粘弹特性,研究基于粘弹假设的数值模拟方法对于正确认识地震波的传播规律和提高地震勘探精度具有重要意义。波动方程正演过程中纵横波的保幅解耦是研究准确的粘弹介质中地震波传播机理的前提,基于散度和旋度算子的纵横波解耦方法会使波场的相位和振幅产生畸变,且解耦后的波场在极性反转位置上无法与分离前混合波场各分量对应。在散度和旋度算子上再做一次梯度和旋度运算的波场分离方法虽然能够克服上述缺陷,但存在保幅性差等问题。本文从粘弹介质中的一阶速度-应力方程出发,推导了矢量纵横波分离的波数域表达式,结合有限差分思路给出了其在空间域的求解方法。本文方法利用纵横波的传播速度对现有的矢量波场分离方法进行振幅校正,并将校正结果分别作为纵波与横波对时间的二阶偏导,实现了粘弹介质中的纵横波分离。模型试算结果表明,本文方法能够克服现有方法的缺陷,获得更具保幅性的波场分离结果。  相似文献   

Isotope Characteristics of Carbonates from Rocks of Greenstone Belts as an Indicator of a Possible Source of Fluids in Precambrian Granulite Complexes: An Example from the Giyani Greenstone Belt and the Limpopo Granulite Complex,South Africa     

Mityaev  A. S.  Safonov  O. G.  Reutsky  V. N.  Izokh  O. P.  Varlamov  D. A.  Kozlovskii  V. M.  van Reenen  D. D.  Aranovich  L. Y. 《Doklady Earth Sciences》2020,492(1):342-345

Doklady Earth Sciences - Data on the carbon and oxygen isotopic composition of carbonates from the rocks of the Giyani greenstone belt, Kaapvaal craton, South Africa are presented. This belt is...  相似文献   

Geophysical signature of the Tunnunik impact structure,Northwest Territories,Canada     

Y. Quesnel  W. Zylberman  P. Rochette  M. Uehara  J. Gattacceca  G. R. Osinski  P. Dussouillez  C. Lepaulard  C. Champollion 《Meteoritics & planetary science》2020,55(3):480-495

In 2011, the discovery of shatter cones confirmed the 28 km diameter Tunnunik complex impact structure, Northwest Territories, Canada. This study presents the first results of ground‐based electromagnetic, gravimetric, and magnetic surveys over this impact structure. Its central area is characterized by a ~10 km wide negative gravity anomaly of about 3 mGal amplitude, roughly corresponding to the area of shatter cones, and associated with a positive magnetic field anomaly of ~120 nT amplitude and 3 km wavelength. The latter correlates well with the location of the deepest uplifted strata, an impact‐tilted Proterozoic dolomite layer of the Shaler Supergroup exposed near the center of the structure and intruded by dolerite dykes. Locally, electromagnetic field data unveil a conductive superficial formation which corresponds to an 80–100 m thick sand layer covering the impact structure. Based on the measurements of magnetic properties of rock samples, we model the source of the magnetic anomaly as the magnetic sediments of the Shaler Supergroup combined with a core of uplifted crystalline basement with enhanced magnetization. More classically, the low gravity signature is attributed to a reduction in density measured on the brecciated target rocks and to the isolated sand formations. However, the present‐day fractured zone does not extend deeper than ~1 km in our model, indicating a possible 1.5 km of erosion since the time of impact, about 430 Ma ago.  相似文献   

hairy和hedgehog在单环刺蜢幼虫体节形成过程中的表达特征分析     

李琦  秦贞奎  张婷婷  魏茂凯  侯西坦  张志峰 《中国海洋大学学报(自然科学版)》2020,50(4):63-69

hairy作为成对控制基因参与果蝇等体节动物的体节形成;体节极性基因hedgehog是节肢动物和环节动物体节边界维持的关键基因。本研究分析了单环刺螠hairy的序列特征以及hairy和hedgehog在其幼虫体节发生过程中的时空表达特征,结果显示:单环刺螠Hairy序列中含有保守的HLH结构域、Hairy_orange结构域和四肽WRPW;其mRNA在早期体节幼虫中的表达量显著高于晚期担轮幼虫,并且定位于每个体节的边界处。单环刺螠hedgehog mRNA在体节幼虫中的表达水平显著高于早期体节幼虫,并且呈现保守的体节边界表达特征。研究结果表明,hairy和hedgehog在单环刺螠幼虫体节中的表达图式与小头虫等典型体节动物中的表达图式基本一致。  相似文献   

四川盆地杂卤石地球物理响应特征及预测方法研究——以川中广安地区为例     

侯学文  李进  余中美  刘君豪  谭志远  熊鸿鸽  张永恒 《盐湖研究》2021,29(1):33-43

川中南充盐盆是四川盆地最大的次一级含盐盆地,区域内钾盐具有成盐厚度大、分布范围广、埋藏深度深、岩性复杂等特点,目前尚未建立一套适用于研究区的钾盐地球物理评价方法。以地球物理勘探原理为基础,结合测井、录井、地质、地震等资料,分析和总结出不同岩性的测井响应特征以及分布范围,根据杂卤石"三高一低"的特点,建立杂卤石测井识别方法。在此基础上,优选伽马和声波速度作为敏感参数,建立了杂卤石的地质—测井—地震三位一体井约束地震反演识别方法,并以广参1井为例,预测杂卤石的空间展布情况。最后结合地震反演结果圈定出广安地区为杂卤石沉积的最有利区域。在实际应用中总结出一套适用于研究区的杂卤石预测方法,为研究区后续勘探开发提供了借鉴与参考,具有一定的推广应用价值。  相似文献   

Stress distribution from railway track over geogrid reinforced ballast underlain by clay     

Fattah  Mohammed Y.  Mahmood  Mahmood R.  Aswad  Mohammed F. 《地震工程与工程振动(英文版)》2019,18(1):77-93

Railway ballast forms a major component of a conventional rail track and is used to distribute the load to the subgrade, providing a smooth running surface for trains. It plays a significant role in providing support for the rail track base and distributing the load to the weaker layer underneath. Ballast also helps with drainage, which is an important factor for any type of transportation structure, including railroads. Over time, ballast progressively deforms and degrades under dynamic loading and loses its strength. In this study, extensive laboratory tests were conducted to investigate the effect of load amplitude, geogrid position, and number of geogrid layers, thickness of ballast layer and clay stiffness on the behavior of the reinforced ballast layer and induced strains in a geogrid. A half full-scale railway was constructed for carrying out the tests, which consisted of two rails 800 mm in length with three wooden sleepers(900 mm × 10 mm × 10 mm). Three ballast thicknesses of 200, 300 and 400 mm were used in the tests. The ballast was overlying 500 mm thickness clay in two states, soft and stiff. The tests were carried out with and without geogrid reinforcement; the tests were performed in a well-tied steel box of 1.5 m length ×1 m width ×1 m height. Laboratory tests were conducted to investigate the response of the ballast and the clay layers where the ballast was reinforced by a geogrid. Settlement in ballast and clay, soil pressure and pore water pressure induced in the clay were measured in reinforced and unreinforced ballast cases. It was concluded that the amount of settlement increased as the simulated train load amplitude increased, and there was a sharp increase in settlement up to cycle 500. After that, there was a gradual increase that leveled out between, 2500 to 4500 cycles depending on the frequency used. There was a slight increase in the induced settlement when the load amplitude increased from 0.5 to 1 ton but it was higher when the load amplitude increased to 2 tons. The increased amount in settlement depended on the existence of the geogrid and other parameters studied. The transmitted average vertical stress for ballast thicknesses of 30 cm and 40 cm increased as the load amplitude increased, regardless of the ballast reinforcement for both soft and stiff clay. The position of the geogrid had no significant effect on the transmitted stresses. The value of the soil pressure and pore water pressure on ballast thicknesses of 20 cm was higher than for 30 cm and 40 cm thicknesses. This meant that the ballast attenuated the induced waves. The soil pressure and pore water pressure for reinforced and unreinforced ballast was higher in stiff clay than in soft clay.  相似文献   

Carbonaceous chondrites as analogs for the composition and alteration of Ceres          下载免费PDF全文

Harry Y. McSween Jr.  Joshua P. Emery  Andrew S. Rivkin  Michael J. Toplis  Julie C. Castillo‐Rogez  Thomas H. Prettyman  M. Cristina De Sanctis  Carle M. Pieters  Carol A. Raymond  Christopher T. Russell 《Meteoritics & planetary science》2018,53(9):1793-1804

The mineralogy and geochemistry of Ceres, as constrained by Dawn's instruments, are broadly consistent with a carbonaceous chondrite (CM/CI) bulk composition. Differences explainable by Ceres’s more advanced alteration include the formation of Mg‐rich serpentine and ammoniated clay; a greater proportion of carbonate and lesser organic matter; amounts of magnetite, sulfide, and carbon that could act as spectral darkening agents; and partial fractionation of water ice and silicates in the interior and regolith. Ceres is not spectrally unique, but is similar to a few other C‐class asteroids, which may also have suffered extensive alteration. All these bodies are among the largest carbonaceous chondrite asteroids, and they orbit in the same part of the Main Belt. Thus, the degree of alteration is apparently related to the size of the body. Although the ammonia now incorporated into clay likely condensed in the outer nebula, we cannot presently determine whether Ceres itself formed in the outer solar system and migrated inward or was assembled within the Main Belt, along with other carbonaceous chondrite bodies.  相似文献