Harvard Seismology: Inner Core Anisotropy

The Earth's inner core has this remarkable property: Compressional waves travel faster along its spin axis than in the equatorial plane. Such a directional dependence of wave propogation, together with the anomalous splitting of core-sensitive normal modes, was explained by an anisotropic inner core model first proposed by Harvard Seismology Group in 1986. Since then, we have further investigated its anisotropy extensively using both travel-time anomalies and the normal modes splitting. The symmetry axis of the anisotropy was used as a marker to detect the differential rotation of the inner core relative to the mantle. Our present research focuses on resolving the three-dimensionality and temporal variation of the anisotropy.

Active participants in this project are Miaki Ishii , Adam Dziewonski, and Wei-jia Su.

Previously active participants in these projects are Jeroen Tromp, and Hong Ma.


Recent Developments


Publications


Miaki Ishii, Department of Earth and Planetary Science, Harvard University, copyright ©1997, all rights reserved
Last modified: February 18, 2002.