AxiSEM3D - an introduction to using the code and its applications

This is a Preprint and has not been peer reviewed. This is version 2 of this Preprint.

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Authors

Benjamin Fernando , Jonathan Wolf , Kuangdai Leng, Tarje Nissen-Meyer, Will Eaton, Marshall Styczinski, Andrew Walker , Timothy J Craig, Jack Muir, Ceri Nunn, Maureen Long

Abstract

Welcome to the wonderful world of AxiSEM3D, a flexible, high-performance computational method for solving the elastodynamic wave equation in three-dimensional, hetereogeneous media. It has been used in seismology for the Earth, the Sun, the Moon, and many of other rocky planets and moons of the Solar System. In this manual, we will explore the practicalities of using this code, touching on the mathematical aspects as relevant to the casual user, the input and output files, and pre- and post-processing. This guide is not a replacement for any of the AxiSEM3D papers, which you will find listed in the next section. Nor does it go into any detail about how to install, build, configure, or make the code as these are dealt with in a separate installation guide. However, it does contain everything to do with the scientific aspects of the code and the user interface post-installation.

DOI

https://doi.org/10.31223/X5TH7P

Subjects

Geophysics and Seismology, Planetary Geophysics and Seismology

Keywords

seismic modelling, AxiSEM3D

Dates

Published: 2024-03-19 10:06

Last Updated: 2024-06-17 21:45

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License

CC-By Attribution-NonCommercial-NoDerivatives 4.0 International

Additional Metadata

Data Availability (Reason not available):
All codes are available either inline or linked to on the relevant GitHub (these are in development and rapidly changing, a repository is not appropriate for in-dev source code at this time).