首页> 外文期刊>Pure and Applied Geophysics >Sediment thicknesses and Q(s) vs. Q(p) relations in the Kachchh rift basin, Gujarat, India using Sp converted phases
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Sediment thicknesses and Q(s) vs. Q(p) relations in the Kachchh rift basin, Gujarat, India using Sp converted phases

机译:印度古吉拉特邦Kachchh裂谷盆地沉积物厚度以及Q(s)与Q(p)关系(采用Sp转换相)

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Delineation of the top sedimentary structure and its Q(s) vs. Q(p) relationship using the travel-time difference of direct S and converted Sp phase is key to understanding the seismic hazard of any sedimentary basin area. We constructed filtered displacement waveforms from local ETNA Episensor acceleration recordings as well as local velocity recordings of aftershocks of the 2001 Bhuj earthquake recorded by the Kachchh seismological network of the National Geophysical Research Institute (NGRI), Hyderabad, India during 2001-2004. Stations are within 15-70km of epicenters, and the resulting displacement waveforms are generally simple, displaying prominent P, Sp, and S wave pulses. Particle motion of P and S waves suggest near-vertical raypaths consistent with preliminary depth estimates. The direct S wave on the horizontal component is characterized by lower frequency content than the converted Sp phase on the vertical component. This difference in frequency content between S and Sp phases can be explained in terms of different attenuation effects for P and S waves in the unconsolidated sediments. The Sp phase is generated by S-to-P phase conversion at the base of Mesozoic sediments of the Kachchh basin. Travel-time inversion (VELEST) of 2565 P and 2380 S arrivals from 658 well located aftershocks recorded at 8-14 three-component local seismic stations led to 1 D velocity models indicated very slow sediments in the upper 0-2 km depth range (Vp: 2.92 km/s and Vs: 0.90 km/s) and an increasing trend of velocities with depth at 2-40 km depth. The estimated sediment thicknesses beneath 12 accelerograph and 6 seismograph sites from the estimated velocity model and the travel-time difference between S and converted Sp phases reaches a maximum of (1.534 +/- 0.117) km beneath Bandri (near the location of 2001 Bhuj mainshock) and attains a minimum sediment thickness of (0.858 +/- 0.104) km beneath Ramvav and Burudia. The spectral ratios between Sp and S from 159 three-component accelerograms have been used to study seismic wave attenuation in the Kachchh rift basin. The estimated Q(s) vs. Q(p) relations for 12 accelerograph sites vary from Q(s) = 0.184 Q(p) (at Chobari) to Q(s) = 0.505 Q(p) (at Dudhai). For stations Chobari, Chopdwa, Jahawarnagar, Vondh and Tapar, the spectral ratio slopes and hence the calculated Q(s) vs. Q(p) relations are effectively the same, and the correlation coefficients are quite high (0.91-0.93). Stations Adhoi, Manfara, New Dudhai, Dudhai and Sikara have similar Q(s) vs. Q(p) relationships to each other and also have high correlation coefficients (0.78-0.87). The spectral ratios for stations Anjar and Ramvav are small and poorly constrained, resulting in less reliable Q(s) vs. Q(p) relations. This could be due to noisy data, fewer available waveforms, or scattering due to velocity heterogeneities and/or interface irregularities.
机译:利用直接S相和Sp转换后相的传播时间差来描述顶部沉积结构及其Q(s)与Q(p)关系是了解任何沉积盆地地区地震危险的关键。我们从2001年至2004年期间印度海得拉巴国家地球物理研究所(NGRI)的卡奇地震波网记录的ETNA Episensor局部加速度记录以及2001年普吉地震余震的局部速度记录中,构造了滤波后的位移波形。测站位于震中15-70公里以内,产生的位移波形通常很简单,显示出明显的P,Sp和S波脉冲。 P波和S波的质点运动暗示了与初步深度估计值一致的近垂直射线路径。水平分量上的直接S波的特征在于其频率含量低于垂直分量上的转换后的Sp相位。 S和Sp相之间频率含量的这种差异可以用未固结沉积物中P和S波的不同衰减效应来解释。 Sp相是在Kachchh盆地中生代沉积物底部通过S-P相转换而生成的。在8-14个三分量本地地震台站记录的658处余震中的2565 P和2380 S到达的传播时间反演(VELEST)导致一维速度模型表明,在0-2 km深度范围内的沉积物非常缓慢( Vp:2.92 km / s和Vs:0.90 km / s),并且深度在2-40 km处的速度呈上升趋势。根据估计的速度模型,估计的12个加速度计和6个地震仪位置下的沉积物厚度,以及S相和转换后的Sp相之间的传播时间差在Bandri下(在2001 Bhuj主震附近)最大(1.534 +/- 0.117)km。 ),并在Ramvav和Burudia下面获得最小的沉积物厚度(0.858 +/- 0.104)km。 159个三分量加速度图中Sp和S之间的频谱比已用于研究Kachchh裂谷盆地的地震波衰减。 12个加速度计位置的估计Q(s)与Q(p)关系从Q(s)= 0.184 Q(p)(在Chobari)到Q(s)= 0.505 Q(p)(在Dudhai)不等。对于Chobari,Chopdwa,Jahawarnagar,Vondh和Tapar台站,频谱比斜率以及因此计算的Q(s)与Q(p)关系实际上是相同的,并且相关系数非常高(0.91-0.93)。气象站Adhoi,Manfara,New Dudhai,Dudhai和Sikara具有相似的Q(s)与Q(p)关系,并且相关系数也很高(0.78-0.87)。 Anjar和Ramvav台站的频谱比很小,约束性很差,导致可靠的Q(s)与Q(p)关系较差。这可能是由于噪声数据,可用波形较少或由于速度异质性和/或界面不规则性造成的散射。

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