一次强烈火山爆发在大气中产生的次声信号的参数

L. Chernogor
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引用次数: 2

摘要

本文的目的是对圣海伦斯火山爆发产生的次声信号的距离和振幅进行回归分析,拟合其结果,并对一些信号和大气参数进行估计。在0.9 ~ 39 mm距离范围内测量了13个站点St. Helens火山爆发初期产生的爆炸波压力幅值;基于这些数据,我们尝试进行回归分析以拟合振幅和距离。基于次声在波导中传播的假设的回归被认为是最可取的回归。根据对圣海伦斯火山喷发冲击波的观测,估计其冲击波能量为~1016 J,平均能量为~2.3 TW。根据对圣海伦斯火山喷发产生的次声波序列的振幅和持续时间的观测,估计次声波能量和平均功率分别为~1016 J和~2 TW。这两种估计都很一致,但它们与文献中发现的显著不同;后者似乎被高估了。根据回归表达式,得到次声波的穿透深度约为33 Mm,而在其他台站估计次声波的尺度长度接近24 Mm。根据大气湍流衰减系数的理论依赖性,估计了10 - 300 s周期次声波的衰减长度。在20 - 300秒周期内,该值已被证明明显大于由观测确定的值。讨论了次声信号衰减的其他机制(次声能量通过波导壁反射的部分辐射和损失)。与此同时,在小于20 ~ 50 s的周期内,随湍流强度的不同,湍流波动对波的散射导致的波衰减也很明显。并将所得到的回归函数与在大气中传播的其他次声源的相应回归表达式进行了比较。关键词:火山喷发,次声波,冲击波,信号幅度,回归,信号衰减
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Parameters of the Infrasonic Signal Generated in the Atmosphere by a Powerful Volcano Explosion
The purpose of this work is to represent the results of performing regression analysis to fit the distance and the amplitude of the infrasonic signal generated by the explosion of St. Helens volcano, and to estimate a few signal and atmospheric parameters. The pressure amplitude in the explosion wave generated at the beginning of St. Helens volcano eruption was measured at 13 stations in the 0.9 – 39-Mm distance range; based on these data, an attempt has been made to perform a regression analysis to fit amplitude and distance. The regression based on the assumption that the infrasound propagation takes place in a waveguide where it is subject to attenuation is determined to be the most preferable regression. Based on the observations of the shock from the St. Helens volcano eruption, the shock wave energy and mean power have been estimated to be ~1016 J and ~2.3 TW, respectively. Based on the observations of the amplitude and duration of the trains of the infrasonic wave generated by the St. Helens volcano eruption, the infrasonic wave energy and mean power have been estimated to be ~1016 J and ~2 TW, respectively. Both estimates are in good agreement, but they are significantly different from those found in the literature; the latter seem to be overestimated. From the regression expression obtained, the penetration depth of the infrasonic wave is obtained to be about 33 Mm, whereas at other stations this scale length is estimated to be close to 24 Mm. Based on the theoretical dependence of the attenuation coefficient due to atmospheric turbulence, the attenuation length of the infrasound wave has been estimated for infrasound with 10–300-s periods. For 20–300-s periods, this value has been shown to be significantly larger than the values determined from the observations. Other mechanisms for attenuating the infrasonic signal are discussed (the partial radiation of the infrasonic energy through and losses due to the reflection from the waveguide walls). At the same time, the wave attenuation due to their scattering by turbulent fluctuations can be significant for the periods smaller than 20–50 s, depending on the turbulence intensity. Comparison of the regression functions obtained with the corresponding regression expressions for other sources of infrasound waves propagating in the atmosphere has been made. Keywords: volcano eruption, infrasonic wave, shock wave, signal amplitude, regression, signal attenuation
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