Nishida Kiwamu, Montagner Jean-Paul, Kawakatsu Hitoshi
Earthquake Research Institute (ERI), The University of Tokyo, 1-1-1, Yayoi, Bunkyo-ku, Tokyo, Japan.
Science. 2009 Oct 2;326(5949):112. doi: 10.1126/science.1176389.
The development of global surface wave tomography using earthquakes has been crucial to exploration of the dynamic status of Earth's deep. It is naturally believed that only large earthquakes can generate long-period seismic waves that penetrate deep enough into Earth for such exploration. The discovery of seismic hum, Earth's background free oscillations, which are randomly generated by oceanic and/or atmospheric disturbances, now provides an alternative approach. We present results of global upper-mantle seismic tomography using seismic hum and without referring to earthquakes. At periods of 100 to 400 seconds, the phase-velocity anomalies of Rayleigh waves are measured by modeling the observed cross-correlation functions between every pair of stations from among 54 globally distributed seismic stations. The anomalies are then inverted to obtain the three-dimensional S-wave velocity structure in the upper mantle. Our technique provides a new means for exploring the three-dimensional structure of the interior of terrestrial planets with an atmosphere and/or oceans, particularly Mars.
利用地震开展全球面波层析成像对于探索地球深部的动力学状态至关重要。人们自然而然地认为,只有大地震才能产生能穿透地球足够深度以供此类探索的长周期地震波。如今,由海洋和/或大气扰动随机产生的地球背景自由振荡——地震嗡鸣的发现,提供了一种替代方法。我们展示了不参考地震数据、利用地震嗡鸣进行全球上地幔地震层析成像的结果。在100至400秒的周期内,通过对全球分布的54个地震台站中每对台站间观测到的互相关函数进行建模,测量瑞利波的相速度异常。然后对这些异常进行反演,以获得上地幔的三维S波速度结构。我们的技术为探索有大气层和/或海洋的类地行星(特别是火星)内部的三维结构提供了一种新手段。