Traveltime delay and initial phase reversal of distant tsunamis coupled with the self-gravitating elastic Earth

Traveltime delay and initial phase reversal of distant tsunamis coupled with the self-gravitating elastic Earth

Shingo Watada1, Satoshi Kusumoto1,2, and Kenji Satake1

Journal of Geophysical Research, 119, 4287-4310, doi:10.1002/2013JB10841.

Abstract

Systematic tsunami traveltime delays of up to 15 min relative to the numerically simulated long waves from the 2010 Chilean and 2011 Tohoku-Oki earthquakes were widely observed at deep ocean tsunamimeters. Enigmatic small negative phases appearing before the main peak were commonly found only at the trans-oceanic locations. The frequency dependence of the measured tsunami phase velocities shows reverse dispersions at long periods, i.e., the tsunami speed becomes slower at periods beyond 1000s. This is consistent with the phase velocities of a tsunami mode coupled with a self-gravitating elastic Earth, suggesting that the effects of compression and dilatation of seawater, elastic tsunami loadings on a solid Earth, and the geopotential variations associated with the motion of mass during tsunami propagation are responsible for the traveltime delays and the initial negative phases. Simple 1-D tsunami propagation tests confirm that the reverse dispersion creates a small negative phase that precedes the main peak at large distances. A new method to simulate tsunami waveforms on real ocean bathymetry that takes into account seawater compressibility, the elasticity of the Earth, and geopotential perturbations has been developed by applying a phase correction to the simulated long waves. The simulated waveforms, in which phase corrections are applied for the dispersion effects, accurately reproduce the observed waveforms, including a small initial negative phase that appears at distant locations. The travel time difference between the observed and simulated waveforms has been decreased to less than 5 min and the waveform difference between them remarkably diminishes.

図1(左)2010年チリ地震と2011年東北地方太平洋沖地震の震源(黄色星)から太平洋を横断して深海のブイ式海底津波計(赤三角)に到達する津波を黒い曲線で描いています。(右)ブイ式海底津波計で観測された津波波形と実際の海底地形と地震断層モデルから計算された津波波形を比較しています。これまでの遠地津波の計算手法による津波波形(青線)に比べ、観測波形(黒線)は遅れて到達し、初動が引き波となっています。今回新たに開発された簡便な計算手法による津波波形(赤線)では観測波形の遅れはほぼ解消し、初動を含めた波形が良く再現できています。