Bayesian inference for ultralow velocity zones in the Earth's lowermost mantle: complex ULVZ beneath the east of the Philippines

dc.contributor.authorPachhai, S.
dc.contributor.authorTkalčić, Hrvoje
dc.contributor.authorDettmer, J.
dc.date.accessioned2015-06-18T04:05:00Z
dc.date.available2015-06-18T04:05:00Z
dc.date.issued2014-11-21
dc.date.updated2015-12-11T09:24:58Z
dc.description.abstractUltralow velocity zones (ULVZs) are small-scale structures with a sharp decrease in S and P wave velocity, and an increase in the density on the top of the Earth's core-mantle boundary. The ratio of S and P wave velocity reduction and density anomaly are important to understanding whether ULVZs consist of partial melt or chemically distinct material. However, existing methods such as forward waveform modeling that utilize 1-D and 2-D Earth-structure models face challenges when trying to uniquely quantify ULVZ properties because of inherent nonuniqueness and nonlinearity. This paper develops a Bayesian inversion for ULVZ parameters and uncertainties with rigorous noise treatment to address these challenges. The posterior probability density of the ULVZ parameters (the solution to the inverse problem) is sampled by the Metropolis-Hastings algorithm. To improve sampling efficiency, parallel tempering is applied by simulating a sequence of tempered Markov chains in parallel and allowing information exchange between chains. First, the Bayesian inversion is applied to simulated noisy data for a realistic ULVZ model. Then, measured data sampling the lowermost mantle under the Philippine Sea are considered. Cluster analysis and visual waveform inspection suggest that two distinct classes of ScP (S waves converted to, and reflected as, P waves) waves exist in this region. The distinct waves likely correspond to lateral variability in the lowermost mantle properties in a NE-SW direction. For the NE area, Bayesian model selection identifies a two-layer model with a gradual density increase as a function of depth as optimal. This complex ULVZ structure can be due to the percolation of iron-enriched, molten material in the lowermost mantle. The results for the SW area are more difficult to interpret, which may be due to the limited number of data available (too few waveforms to appropriately reduce noise) and/or complex 2-D and 3-D structures that cannot be explained properly by the 1-D models required by our inversion approach. In particular, the complex waveforms require highly layered 1-D models to fit the data. These models appear physically unreasonable and suggest that the SW region cannot be explained by 1-D structure.
dc.description.sponsorshipNational Collaborative Research Infrastructure Strategy (NCRIS) and the Education Investment Fund (EIF3).en_AU
dc.identifier.issn2169-9313en_AU
dc.identifier.urihttp://hdl.handle.net/1885/14002
dc.publisherWiley
dc.rights© 2014. American Geophysical Union. http://publications.agu.org/author-resource-center/usage-permissions/#repository..."AGU allows authors to deposit their journal articles if the version is the final published citable version of record, the AGU copyright statement is clearly visible on the posting, and the posting is made 6 months after official publication by the AGU." from the publisher website as at 18/06/15.
dc.sourceJournal of Geophysical Research: Solid Earth
dc.titleBayesian inference for ultralow velocity zones in the Earth's lowermost mantle: complex ULVZ beneath the east of the Philippines
dc.typeJournal article
dcterms.dateAccepted2014-10-22
local.bibliographicCitation.issue11en_AU
local.bibliographicCitation.lastpage8365en_AU
local.bibliographicCitation.startpage8346en_AU
local.contributor.affiliationPachhai, S.,en_AU
local.contributor.authoremailsurya.pachhai@anu.edu.auen_AU
local.contributor.authoruidu4923660en_AU
local.identifier.absfor040407 - Seismology and Seismic Exploration
local.identifier.absseo970104 - Expanding Knowledge in the Earth Sciences
local.identifier.ariespublicationU3488905xPUB5176
local.identifier.citationvolume119en_AU
local.identifier.doi10.1002/2014JB011067en_AU
local.identifier.scopusID2-s2.0-84919467095
local.identifier.thomsonID000346656100019
local.identifier.uidSubmittedByu1005913en_AU
local.publisher.urlhttp://au.wiley.com/WileyCDA/en_AU
local.type.statusPublished Versionen_AU

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