Journal article
Inference of the S- to P-wave velocity anomalies ratio and its uncertainty with an application to South-East Asia
- Abstract:
- The ratio R of shear-wave to compressional-wave velocity variations (dlnVs/dlnVp) is a useful physical parameter to study the thermochemical properties of the Earth’s interior. Several approaches have been employed to estimate R (or its inverse 1/R), but they either assume the same local resolution in models of dlnVs and dlnVp or assume the same ray paths for S- and P-phases, while excluding valuable data and overlooking uncertainties. We overcome these issues by characterizing both dlnVs and dlnVp through the Backus-Gilbert based subtractive optimally localized averages (SOLA) method to obtain R including its uncertainties. This approach enables us to ensure that dlnVs and dlnVp share the same local resolution, making it possible to compute their ratio through division. In addition, SOLA provides uncertainties on dlnVs and dlnVp, which we propagate into our estimates of R using the Hinkley distribution for dlnVs/dlnVp. When resembling a Gaussian, the Hinkley distribution provides Gaussian uncertainties for R, enabling us to interpret tomographic features as, for instance, in terms of slab morphology or partial melt with greater confidence. To illustrate our new approach, we use a data set of P- and S-phase onset-time residuals from ISC to infer the velocity anomalies and the ratio R (or 1/R) in South-East Asia between 100 and 800 km depth. As the SOLA method is driven by data uncertainties, we reassess the provided ISC uncertainties using a statistical approach before developing models of dlnVs and dlnVp with their uncertainties. Based on our quantitative model estimates, we argue that a large velocity anomaly below the Sumatra slab, with a value of R over 2.5, is resolved given our data and their uncertainties. However, in contrast to previous work, we do not find evidence for a slab hole under Java. Our proposed approach to obtain R with uncertainties using the Hinkley distribution can be applied to a large range of tomographic imaging settings
- Publication status:
- Published
- Peer review status:
- Peer reviewed
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(Preview, Version of record, pdf, 3.1MB, Terms of use)
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(Preview, Supplementary materials, pdf, 36.6MB, Terms of use)
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- Publisher copy:
- 10.1093/gji/ggaf468
Authors
+ Royal Society
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- Funder identifier:
- https://ror.org/03wnrjx87
- Grant:
- URF\R1\180377
- URF\R\241025
- Publisher:
- Oxford University Press
- Journal:
- Geophysical Journal International More from this journal
- Volume:
- 244
- Issue:
- 1
- Article number:
- ggaf468
- Publication date:
- 2025-11-18
- Acceptance date:
- 2025-11-11
- DOI:
- EISSN:
-
1365-246X
- ISSN:
-
0956-540X
- Language:
-
English
- Keywords:
- Pubs id:
-
2324526
- Local pid:
-
pubs:2324526
- Deposit date:
-
2025-11-12
- ARK identifier:
Terms of use
- Copyright holder:
- Serra et al.
- Copyright date:
- 2025
- Rights statement:
- ©The Author(s) 2025. Published by Oxford University Press on behalf of The Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.
- Licence:
- CC Attribution (CC BY)
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