Finite Frequency P-Wave Tomography for French Polynesian Region

Tuesday, 16 December 2014
Masayuki Obayashi1, Junko Yoshimitsu1, Hiroko Sugioka1, Aki Ito1, Takehi Isse2, Hajime Shiobara2 and Daisuke Suetsugu1, (1)JAMSTEC, D-EARTH, Yokosuka, Japan, (2)University of Tokyo, Bunkyo-ku, Japan
The French Polynesian region is characterized by positive topographic anomalies of 700 m, a concentration of hotspot chains. Many seismic tomography results show a broad low-velocity anomaly in the lower mantle continued from the base of the mantle. These observations suggest that a large-scale mantle flow rises from the bottom of the mantle beneath the region. Joint Japanese-French broadband seismological observations were performed from 2001 to 2005 with 10 island stations from the Polynesian PLUME project and 10 broadband ocean bottom seismometers (BBOBSs) from the Polynesian BBOBS project. A P-wave tomography using the data from these projects revealed that large-scale low-velocity anomalies (on the order of 1000 km in diameter) from the bottom of the mantle become smaller-scale low-velocity anomalies (on the order of 100 km in diameter) at the depth of about 1000 km. However the connection of the small-scale low-velocity anomalies to the surface hotspots was not unrevealed because of the poor resolution in the upper mantle.

A new P-wave tomography with better resolution in the upper mantle was obtained by adding data from BBOSBSs around Society Islands deployed along the TIARES project during 2009 - 2010 and by taking the finite frequency effect into account for the frequency-depended differential travel times. The frequency-depended differential travel times were measured by multi-band cross correlating P waveforms. The new P-wave tomography shows strong low-velocity anomalies beneath the Society Islands and Pitcairn in the upper mantle although they do not extend to the 660-km discontinuity. This model also shows that small-scale low-velocity anomalies in the uppermost lower mantle. The low-velocity anomalies in the depth range about 550 - 900 km are smaller both in lateral area and amplitude than those in most of the upper mantle and the lower mantle. There is no correlation between velocity patterns in that depth range and those in the upper mantle or in the lower mantle, suggesting that the broad slow anomalies in the lower mantle do not connect to the surface directly.