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991.
In the framework of the French-Ivorian participation to the IEEY, a network of 10 electromagnetic stations were installed at African longitudes. The aim of this experiment was twofold: firstly, to study the magnetic signature of the equatorial electrojet on the one hand, and secondly, to characterize the induced electric field variations on the other hand. The first results of the magnetic field investigations were presented by Doumouya and coworkers. Those of the electric field experiment will be discussed in this study. The electromagnetic experiment will be described. The analysis of the electromagnetic transient variations was conducted in accordance with the classical distinction between quiet and disturbed magnetic situations. A morphological analysis of the recordings is given, taking into consideration successively quiet and disturbed magnetic situations, with the results interpreted in terms of the characterization of external and internal sources. Particular attention was paid to the effects of the source characteristics on the induced field of internal origin, and to the bias they may consequently cause to the results of electromagnetic probing of the Earth; the source effect in electromagnetic induction studies. During quiet magnetic situations, our results demonstrated the existence of two different sources. One of these, the SRE source, was responsible for most of the magnetic diurnal variation and corresponded to the well-known magnetic signature of the equatorial electrojet. The other source (the SR*E source) was responsible for most of the electric diurnal variation, and was also likely to be an ionospheric source. Electric and magnetic diurnal variations are therefore related to different ionospheric sources, and interpreting the electric diurnal variation as induced by the magnetic field diurnal variation is not relevant. Furthermore, the magnetotelluric probing of the upper mantle at dip equator latitudes with the electromagnetic diurnal variation is consequently impossible to perform. In the case of irregular variations, the source effect related to the equatorial electrojet is also discussed. A Gaussian model of equatorial electrojet was considered, and apparent resistivities were computed for two models of stratified Earth corresponding to the average resistive structure of the two tectonic provinces crossed by the profile: a sedimentary basin and a cratonic shield. The apparent resistivity curves were found to depend significantly on both the model used and the distance to the center of the electrojet. These numerical results confirm the existence of a daytime source effect related to the equatorial electrojet. Furthermore, we show that the results account for the observed differences between daytime and night-time apparent resistivity curves. In particular, it was shown that electromagnetic probing of the Earth using the classical Cagniard-Tikhonov magnetotelluric method is impossible with daytime recordings made at dip latitude stations.  相似文献   
992.
磁暴二倍法预报唐山7.8级地震   总被引:5,自引:0,他引:5       下载免费PDF全文
磁暴二倍法预报地震的依据是,应变能在运移过程中导致地壳膨胀和压缩形成一个周期,在时间上呈有二倍关系.唐山7.8级地震是我国70年代最大地震,用磁暴二倍法推出有4组磁暴能对应这次地震.每组磁暴前后都发生了地震,由于这些地震释放的剩余能量在聚积过程中,地壳发生膨胀和压缩,地磁场就受到影响形成了磁暴.因此磁暴与地震能量变化有相关性.可见,磁暴二倍法可以预报地震.  相似文献   
993.
本文介绍了三榀钢支撑钢筋混凝土框架结构(包括两榀复合耗能支撑框架、一榀普通支撑框架)在低周反复荷载作用下的试验结果。对复合耗能支撑框架结构在低周反复荷载作用下的工作性能(包括受力性能、破坏形态、滞回曲线、骨架曲线、延性和耗能能力等)进行了探讨,揭示了复合耗能支撑框架结构良好的抗震性能。  相似文献   
994.
THREEKINDSOFTIMEDISTRIBUTIONFUNCTIONSOFREMARKABLEEARTHQUAKESINSEISMICSEQUENCESDiaoShouzhongWangHongweiChaoHongtaiHuaAijun(Sei...  相似文献   
995.
StudyonfinestructureofcrustmantletransitionzoneinYanqingHailaibasinbasedonCDPandDSSdataJINCHENG1)(成瑾)QINGHELI2)(李清河)1)In...  相似文献   
996.
新型耗能(阻尼)减震器的开发与研究   总被引:18,自引:7,他引:11  
本文阐述了耗能减震的概念和原理,提出了耗能减震器设计的新思想,研制开发了多种新型实用耗能(阻尼)减震器,并对其中的圆环耗能器、双环耗能器、架颈圆环耗能器、弹塑性-摩擦复合耗能器等进行了循环荷载试验,考察了耗能器代作性能和耗能性能,对已装与未装耗能减震器的钢筋混凝土框架模型进行了伪动力对比实验,进一步考察了耗能减震器的减震效果。在试验研究的基础上,地耗能(阻尼)减震结构体系的分析方法进行了研究,并编  相似文献   
997.
同时满足多个阻尼反应谱的人造地震动时程合成   总被引:1,自引:0,他引:1  
应用M.Hirasawa和M.Watabe(1992)提出的方法,进行了相应的数学推导:即以满足某个阻尼比的反应谱的人造地震动作为初始时程,采用奇异值分解法,通过解线性方程组求出校正时程,并多次叠以逐步辐近  相似文献   
998.
中国地震速报台网走时残差分析与走时修正   总被引:4,自引:0,他引:4  
使用了30个速报台站的观测数据,计算了100多个中国境内外的地震事件初至波走时残差。在此基础上分析各台所记录的所有地震事件的残差随方位角和震中距的分布,及产生这些残差的地球深部非流体静力平衡状态和地球表面构造等方面的原因,并给出了不同区域地震走时的平均校正值,从而提高了地震定位精度。  相似文献   
999.
A procedure is presented for the analysis of complex stationary time series for which the Fourier power spectra reveals broadband noise or broadened pulses. We first determine the Hurst exponent from which we may know whether the time series under study is mainly random or if the data points present correlations. If the data are correlated, a chaotic analysis will reveal whether they may be interpreted as a low dimensional nonlinear system (defined by a low correlation dimension and a finite and positive Kolmogorov entropy and largest positive Lyapunov exponent) or as a stochastic process. We have studied three kind of temporal series: inter-event time series of infrasonic pulses recorded at Stromboli volcano, and, S-coda waves and microseisms, that have been recorded at the eastern Pyrenees. Results show that microseisms and Coda waves can be modeled as a low dimensional deterministic system, Correlation dimensions 2.3, 3.2, respectively. At the contrary infrasonic has resulted stochastic. This chaotic character can be attributed to the medium properties. Coda waves with scattering through a fractal distribution of scatters or to multiple reflection inside resonators (for example sedimentary basins) and microseisms as a propagation of wave guide of variable cross section which have the same temporal characteristics as a nonlinear forced oscillator.  相似文献   
1000.
Space spectral analysis of zonal (u) and meridional (v) components of wind and time spectral analysis of kinetic energy of zonal waves at 850 hPa during monsoon 1991 (1st June 1991 to 31st August 1991) for the global belt between equator and 40°N are investigated. Space spectral analysis shows that long waves (wavenumbers 1 and 2) dominate the energetics of Region 1 (equator to 20°N) while over Region 2 (20°N to 40°N) the kinetic energy of short waves (wavenumbers 3 to 10) is more than kinetic energy of long waves. It has been found that kinetic energy of long waves is dominated by zonal component while both (zonal and meridional) the components of wind have almost equal contribution in the kinetic energy of short waves. Temporal variations of kinetic energy of wavenumber 2 over Region 1 and Region 2 are almost identical. The correlation matrix of different time series shows that (i) wavenumber 2 over Regions 1 and 2 might have the same energy source and (ii) there is a possibility of an exchange of kinetic energy between wavenumber 1 over Region 1 and short waves over Region 2. Wave to wave interactions indicate that short waves over Region 2 are the common source of kinetic energy to wavenumber 2 over Regions 1 and 2 and wavenumber 1 over Region 1. Time spectral analysis of kinetic energy of zonal waves indicates that wavenumber 1 is dominated by 30–45 day and bi-weekly oscillations while short waves are dominated by weekly and bi-weekly oscillations. The correlation matrix, wave to wave interaction and time spectral analysis together suggest that short period oscillations of kinetic energy of wavenumber 1 might be one of the factors causing dominant weekly (5–9 day) and bi-weekly (10–18 day) oscillations in the kinetic energy of short waves.  相似文献   
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