Published March 24, 2025 | Version v1

Evaluating Seismic Ambient Noise Techniques for Detecting Ice-Bearing Rocks on the Moon - Synthetic Data

  • 1. ROR icon Ludwig-Maximilians-Universität München

Contributors

Researcher:

  • 1. ROR icon Ludwig-Maximilians-Universität München

Description

This repository contains all the synthetic data used for the research paper "Evaluating Seismic Ambient Noise Techniques for Detecting Ice-Bearing Rocks on the Moon". The synthetic data were generated with the spectral element code SALVUS (Afanasiev et al., 2019) using a 2D digital twin model of the shallow subsurface structure of the Moon developed by Keil et al. (2024). Different simulation runs were performed with varying parameters of the ice-bearing rock including the weight percent of ice, size and depth. The generated data are in the folder "Synthetic_data". The README.pdf file contains more information on the synthetic data.

 

 

 

Files

README.pdf

Files (2.6 GB)

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Additional details

References

  • Afanasiev, M., Boehm, C., van Driel, M., Krischer, L., Rietmann, M., May, D. A., et al. (2019). Modular and flexible spectral‐element waveform modelling in two and three dimensions. Geophysical Journal International, 216(3), 1675–1692. https://doi.org/10.1093/gji/ggy469
  • Keil,S., Igel,H., Schimmel,M., Lindner,F., & Bernauer,F. (2024). Investigating subsurface properties of the shallow lunar crust using seismic interferometry on synthetic and recorded data. Earth and Space Science, 11(10), e2024EA003742.