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The codes found here calculate receiver function (RF) and perform time to depth migration, in a 3D spherical coordinate system.

We use these codes examine the Moho depth variations for the broader European Alpine region, based on four temporary seismic networks (i.e., AASN, EASI, CIFALPS, PACASE).

For a few more details on this project, have a look at our manuscript entitled “Moho depths beneath the European Alps: a homogeneously processed map and receiver functions database” published at Earth System Science Data (ESSD). The receiver function dataset, we use in the work above is freely available on the following Zenodo repository.

A tutorial for calculating RFs and time-to-depth migrations for a subset of seismic data is available in the documentation.

Documentation is available here.

If you use rfmpy, consider citing Michailos et al. (2023).

Please report bugs, feature requests, and questions through the Issues tracker.

• Michailos, K., Hetényi, G., Scarponi, M., Stipčević, J., Bianchi, I., Bonatto, L., Czuba, W., Di Bona, M., Govoni, A., Hannemann, K., Janik, T., Kalmár, D., Kind, R., Link, F., Lucente, F. P., Monna, S., Montuori, C., Mroczek, S., Paul, A., Piromallo, C., Plomerová, J., Rewers, J., Salimbeni, S., Tilmann, F., Środa, P., Vergne, J., and the AlpArray-PACASE Working Groups, (published at ESSD), 2023.

Please note that, at least at this stage, the codes are designed to reproduce our results. For different applications the codes will need to be modified.

The codes are currently at development and are subject to change at any time. We welcome any code improvements or suggestions and error reports from the community.