Detection of a ULVZ in the Central Pacific using high frequency Sdiff postcursors

Publication date

2024-12-15

Authors

Martin, C.ISNI 0000000524167785
Russell, Stuart
Cottaar, Sanne

Editors

Advisors

Supervisors

Document Type

Article
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cc_by

Abstract

In recent decades, ultra-low velocity zones (ULVZs) – thin patches of strongly reduced seismic velocity atop the core-mantle boundary (CMB) – have been inferred from observations of a variety of seismic phases. One such phase is Sdiff and its out-of-plane postcursory energy, Sdiff+. In this study, we present a high quality dataset of Sdiff and Sdiff+ which shows evidence of a ULVZ in the central Pacific, roughly between Hawaii and Marquesas. The observed Sdiff+ have an unusually short dominant period (5–12 seconds) compared to previous Sdiff+ observations, which is indicative of a ULVZ that is approximately 10–15 km thick. We analyse this high frequency dataset using the 2D Wavefront Tracker (2DWT) Bayesian inversion methodology to generate a probabilistic ensemble of ULVZ models. As a result of the uniazimuthal coverage of data, there is a strong southwest-northeast trade-off, but there is a slight preference for the ULVZ to be located just outside the Pacific large low velocity province (LLVP) boundary, roughly centred 20° north of Marquesas and 20° southeast of Hawaii. The 2DWT inversion of Sdiff+ travel times suggest that the ULVZ can be approximated as a cylindrical structure; either as a larger and weaker anomaly (radius 280 km, dVs -20%) close to the LLVP, or a smaller and stronger anomaly (radius 180 km, dVs -30%) further away from the LLVP. Unlike previous broad-scale ULVZs modelled with Sdiff+, this ULVZ is thinner, might lie outside of an LLVP, and lacks a potential relationship to a mantle plume.

Keywords

Geophysics, Geochemistry and Petrology, Space and Planetary Science, Earth and Planetary Sciences (miscellaneous)

Citation

Martin, C, Russell, S & Cottaar, S 2024, 'Detection of a ULVZ in the Central Pacific using high frequency Sdiff postcursors', Earth and Planetary Science Letters, vol. 648, 119028. https://doi.org/10.1016/j.epsl.2024.119028