山西地堑系一类特殊的剪切-挤压型地裂缝     

宋彦辉  彭建兵  卢全中  李忠生 《工程地质学报》2007,15(4):448-452

阐述了山西地堑系的构造背景及现今应力场状态,对该地区发育的地裂缝特点进行了概括性描述。根据实际调查,在该地区发现了一类特殊的剪切-挤压型地裂缝万荣县城关变电所地裂缝,该地裂缝地貌上位于山西地堑系峨嵋台地,发育特征表现为强烈的剪切、挤压变形,地面、墙体拱曲、翘起,并出现明显的水平位错现象。与该区发育的其他地裂缝有明显的不同。根据地裂缝发育的特征,并结合区域构造应力场分析,讨论了该地裂缝的力学成因机制。  相似文献   

冲绳海槽轴线地质特征   总被引：10，自引：2，他引：10  

杨文达  王振宇  曾久岭 《海洋地质与第四纪地质》2001,21(2):1-6

冲绳海槽位于东海大陆架与琉球岛弧之间，海槽中发育着一系列平行轴向延伸的地堑型正断层。穿越海槽的地震剖面证实了海槽扩张中心的存在，扩张轴沿海槽轴线方向延伸。由于地堑构造中心的扩张速率较大，由某引起的海槽中心下陷的速率大于沉积作用的补偿速率，使海槽中心海底出现明显的下陷。在轴线的大陆坡一侧，陆源沉积占绝对优势；轴线的岛坡一侧，以火山坡碎屑、浮岩、有孔虫软泥为沉积特征。  相似文献   

Rr CrB and Algol – The First and Last Star in Zdeněk Kopal’s Life with Binaries     

Martin Šolc 《Astrophysics and Space Science》2005,296(1-4):43-54

Several important turning points appeared in the personal life and scientific career of Zdeněk Kopal, every time, when he entered a new field of research. Four particular periods of his life will be commented in the present paper: the studies in Prague and early observations in the variable star programme of the Czech Astronomical Society; the first lectures on close binaries at Harvard; the intermezzo of lunar research; and the last period after 1989, when Zdeněk Kopal returned several times to Prague University.  相似文献   

Lunar and solar daily variations of equivalent slab thickness at Delhi   总被引：1，自引：0，他引：1  

P. K. Bhuyan  T. R. Tyagi 《Geophysical Journal International》1987,88(2):487-493

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山西霍山山前断裂晚第四纪活动特征和1303年洪洞8级地震   总被引：25，自引：10，他引：15       下载免费PDF全文

徐锡伟  邓起东 《地震地质》1990,12(1):21-30,T002

霍山山前断裂是山西临汾盆地北半部主边界断裂。本文根据沿断裂带的1:1万地质填图结果,详细地研究了霍山山前断裂的活动历史、断裂的分段性及其构造活动特征、不同时期以来的右旋错动幅度和滑动速率以及与1303年洪洞8级地震的关系。最后,根据山西地堑系内已获得滑动速率值的几条北北东向主干断裂的构造特殊性,讨论了地堑系两侧的一级右旋运动水平  相似文献   

月球辐射照度模型比对及地基对月观测验证     

张璐  张鹏  胡秀清  陈林  王阳  王威 《遥感学报》2017,21(6):864-870

月球是除太阳外对地张角最大的天体,反射率稳定性为10–8每年,适合用于遥感卫星的辐射定标、夜间地基大气遥感和夜间卫星遥感,但月球辐射照度模型的精度束缚了上述应用的发展。为检验现有ROLO(RObotic Lunar Observatory)和MT2009(Miller-Turner 2009)地基整盘月球辐射照度模型的精度,国家卫星气象中心于2015年底至2016年初在云南丽江组织了3个月的地基对月观测,使用高光谱月球成像光谱仪获取了399.00—1060.00 nm连续光谱的月球辐射照度。基于整盘月球辐射照度模型,利用丽江地基对月观测试验资料,对比模型与模型、模型与丽江地基观测月球辐射照度。结果表明:(1)MT2009与ROLO模型在短波红外谱段的差异明显大于可见光谱段;(2)地基观测高光谱月球辐射照度结果与ROLO模型更接近,但是可见光波段比ROLO模型辐射照度平均小5.86%左右。为探究差异产生的主要来源,对结果还进行了进一步的分析和讨论,以期为今后月球辐射模型的改进和夜间微光遥感研究提供经验和依据。  相似文献   

The structural and sedimentological setting of the Quaternary deposits in Al-Ain area, UAE   总被引：1，自引：0，他引：1  

Mohamed A. El-Ghawaby  Mohamed I. El-Sayed 《Journal of Arid Environments》1997,35(4):627-640

Quaternary sediments represent the main constituent which covers an ENE–WSW elongated depression some 25 km long and 10 km wide (Al-Ain area). This depression is encountered between two north and south low fault scarps and is located perpendicular to the Al Jaww plain and Jabel Hafit axes.Four main types of Quaternary surface deposits were identified belonging to: flood plain and braided channels; desert plain; aeolian sand; and sabkha. The first type shows many pedogenic and non-pedogenic features of which are dolocrete, calcrete and gypcrete.An ENE–WSW closely-spaced dip-slip, stepping pattern fault set could be traced in dolocretized-calcretized braided channel deposits, on the south margin of this depression, where the relationship between fault geometry, displacement and geomorphology suggest a model of either graben or half-graben. The role of this system in developing the landscape of Al-Ain is well documented near the surface but a comprehensive study to assess its role in the sub-surface is needed.  相似文献   

山西地堑系强震的活动规律和危险区段的研究   总被引：16，自引：3，他引：16       下载免费PDF全文

徐锡伟  邓起东 《地震地质》1992,14(4):305-316

山西地堑系是我国著名的历史强震活动带之一。作者系统地分析了山西地堑系历史强震的重复和迁移现象、M≥7级地震前中强地震的活动特征、蠕变曲线的线性分段性,并根据近期地震活动的特点,判断了现今地震活动暂态和未来地震活动性;最后,在现有的形变测量资料、历史地震和古地震研究成果的基础上,确定了山西地堑系内可能发生强震的危险区段  相似文献   

海洋和电离层发电机对佘山台L的影响   总被引：1，自引：0，他引：1  

康国发 《地震地磁观测与研究》1992,13(4):46-50

本文在文献[1]的研究基础上进一步分析海洋和电离层发电机对佘山台L的影响。资料分别按月、季节和年以及太阳活动性分组进行的细致分析,结果表明海洋发电机对Z分量的L有一稳定的影响,L的季节变化主要起源于电离层发电机。L的海洋部分不随太阳活动性改变,太阳活动对L的影响比对S的小。  相似文献   

Critical remarks on the use of medieval eclipse records for the determination of long-term changes in the Earth's rotation     

W. Dalmau 《Surveys in Geophysics》1997,18(2-3):213-223

The use of some Arabic medieval solar and lunar eclipse records for the determination of secular changes in the Earth's rotation is critically reviewed. The published results derived from these data suggest a non-uniform decrease in the Earth's rotation rate over the last 27 cy. There is, however, up to this day no sound physical explanation for the deduced non-tidal oscillations, with an apparent period of about 1500 yr and a semi-amplitude of some 4 ms in the l.o.d., which overlayed to a constant secular tidal change in the Earth's rotation rate produce a net non-uniform deceleration of the Earth's rotation. In this paper we discuss a set of observations, which were executed by professional Arabic astronomers. We show by our analysis the way in which the non-uniform deceleration of the Earth's rotation was constructed. A correct reading of the Arabic medieval observations shows that they do not contradict a secular constant decrease in the Earth's rotation rate of nearly -4.6 10-22 rad s-2. This value is in accordance with other similar ones derived from ancient eclipse records and from satellite tracking data.  相似文献