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The mobility of the lithosphere over a weaker asthenosphere constitutes the essential element of plate tectonics, and thus the understanding of the processes at the [ithosphere-asthenosphere boundary (LAB) is fundamental to understand how our planet works. It is especially so for oceanic plates because their relatively simple creation and evolution should enable easy elucidation of the LAB. Data from borehole broadband ocean bottom seismometers show that the LAB beneath the Pacific and Philippine Sea plates is sharp and age-dependent. The observed large shear wave velocity reduction at the LAB requires a partially molten asthenosphere consisting of horizontal melt-rich layers embedded in melt-rich mantle, which accounts for the large viscosity contrast at the LAB that facilitates horizontal plate motions. [ABSTRACT FROM AUTHOR]

High frequency energy radiation of large earthquakes is a key to evaluating shaking damage and is an important source characteristic for understanding rupture dynamics. We developed a new inversion method, Image Deconvolution Back-Projection (IDBP) to retrieve high frequency energy radiation of seismic sources by linear inversion of observed images from a back-projection approach. The observed back-projection image for multiple sources is considered as a convolution of the image of the true radiated energy and the array response for a point source. The array response that spreads energy both in space and time is evaluated by using data of a smaller reference earthquake that can be assumed to be a point source. The synthetic test of the method shows that the spatial and temporal resolution of the source is much better than that for the conventional back-projection method. We applied this new method to the 2001 M w 7.8 Kunlun earthquake using data recorded by Hi-net in Japan. The new method resolves a sharp image of the high frequency energy radiation with a significant portion of supershear rupture. [ABSTRACT FROM AUTHOR]

Abstract: We determined the depths of the 410-km and 660-km seismic discontinuities (called “410” and “660,” respectively, hereafter) beneath the Philippine Sea and the northwestern Pacific by the receiver function method; we used the broadband data obtained from broadband ocean-bottom seismographs. We found a very deep “660” at 691km in the stagnant slab beneath the Philippine Sea. In the surrounding Philippine Sea regions and northwestern Pacific, the “660” appears at depths of 659–674km. Comparison of the “660” depth and P-velocity anomalies indicated that temperatures in the stagnant slab are lower than that in the mantle transition zone (MTZ) beneath the northwestern Pacific by about 500K. The temperature in the MTZ beneath the Parece Vela Basin and West Philippine Sea Basin, which surrounds the stagnant slab, is lower than that in the MTZ beneath the Pacific by about 200K. The water content in the stagnant slab (∼0.2wt% H2O) is higher than that in the other regions; however, the large uncertainty in the estimated water content (±0.2–0.3wt% H2O) prevents us from arriving at a definitive conclusion regarding the presence of water in the stagnant slab. Therefore, it is desirable to use other geophysical parameters (e.g., electrical conductivity) along with the seismic parameters in order to obtain an accurate estimate of the water content in the MTZ. [ABSTRACT FROM AUTHOR]