Please use this identifier to cite or link to this item: https://hdl.handle.net/10356/163899
Title: 3D transdimensional seismic tomography of the inner core
Authors: Brett, Henry
Hawkins, Rhy
Waszek, Lauren
Lythgoe, Karen
Deuss, Arwen
Keywords: Science::Geology
Issue Date: 2022
Source: Brett, H., Hawkins, R., Waszek, L., Lythgoe, K. & Deuss, A. (2022). 3D transdimensional seismic tomography of the inner core. Earth and Planetary Science Letters, 593, 117688-. https://dx.doi.org/10.1016/j.epsl.2022.117688
Journal: Earth and Planetary Science Letters 
Abstract: Body wave observations of the Earth's inner core show that it contains strong seismic heterogeneity, both laterally and radially. Models of inner core structure generated using body wave data are often limited by their parameterisation. Thus, it is difficult to determine whether features such as anisotropic hemispheres or an innermost inner core truly exist with their simple shapes, or result only from the chosen parameterisation and are in fact more complex features. To overcome this limitation, we conduct seismic tomography using transdimensional Markov Chain Monte Carlo on a high quality dataset of 5296 differential and 2344 absolute P-wave travel times. In a transdimensional approach, the data defines the model space parameterisation, providing us with both the mean value of each model parameter and its probability distribution, allowing us to identify well versus poorly constrained regions. We robustly recover many first order observations found in previous studies without the imposition of a priori fixed geometry including an isotropic top layer (with anisotropy less than 1%) which is between 60 and 170 km thick, and separated into hemispheres with a slow west and a faster east. Strong anisotropy (with a maximum of 7.2%) is found mainly in the west, with much weaker anisotropy in the east. We observe for the first time that the western anisotropic zone is largely confined to the northern hemisphere, a property which would not be recognised in models assuming a simple hemispherical parameterisation. We further find that the inner most inner core, in which the slowest anisotropic velocity direction is tilted relative to Earth's axis of rotation (ζ=55∘±16∘), is offset by 400 km from the centre of the inner core and is restricted to the eastern hemisphere. We propose that this anomalous anisotropy might indicate the presence of a different phase of iron (either bcc or fcc) compared to the rest of the inner core (hcp).
URI: https://hdl.handle.net/10356/163899
ISSN: 0012-821X
DOI: 10.1016/j.epsl.2022.117688
Rights: © 2022 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).
Fulltext Permission: open
Fulltext Availability: With Fulltext
Appears in Collections:EOS Journal Articles

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