Solving the eikonal equation for compressional and shear waves in anisotropic media using peridynamic differential operator
Affiliation
Department of Aerospace and Mechanical Engineering, The University of ArizonaIssue Date
2022
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Oxford University PressCitation
Bekar, A. C., Madenci, E., Haghighat, E., Waheed, U. B., & Alkhalifah, T. (2022). Solving the eikonal equation for compressional and shear waves in anisotropic media using peridynamic differential operator. Geophysical Journal International.Rights
Copyright © The Author(s) 2022. Published by Oxford University Press on behalf of The Royal Astronomical Society.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
Traveltimes of compressional (P) and shear (S) waves have proven essential in many earthquake and exploration seismology applications. An accurate and efficient traveltime computation for P and S waves is crucial for the success of these applications. However, solving the eikonal equation with a complex phase velocity field in anisotropic media is challenging. The eikonal equation is a first-order nonlinear hyperbolic partial differential equation. It represents the high-frequency asymptotic approximation of the wave equation. The fast marching and sweeping methods are commonly used due to their efficiency in numerically solving the eikonal equation. However, these methods suffer from numerical inaccuracy in anisotropic media with sharp heterogeneity, irregular surface topography and complex phase velocity fields. This study presents a new method for the solution of the eikonal equation by employing the peridynamic differential operator (PDDO). The PDDO provides the non-local form of the eikonal equation by introducing an internal length parameter (horizon) and a weight function with directional non-locality. The operator is immune to discontinuities in the form of sharp changes in field or model variables and invokes the direction of traveltime in a consistent manner. The weight function controls the strength of association among points within the horizon. Solutions are constructed in a consistent manner without upwind assumptions through simple discretization. The robustness of this approach is established by considering different types of eikonal equations on complex velocity models in anisotropic media. The examples demonstrate its unconditional numerical stability and results compare well with the reference solutions. © 2022 The Author(s) 2022. Published by Oxford University Press on behalf of The Royal Astronomical Society.Note
Immediate accessISSN
0956-540XVersion
Final published versionae974a485f413a2113503eed53cd6c53
10.1093/gji/ggac037