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Adobe PDF - 2.8 MB - MD5: 95f25986c8ebacf2c435fe1cea421605
Article figure 5
Adobe PDF - 18.6 KB - MD5: 0dea6792a6502dba042d9fcde9f63929
Orientation distribution from steep slopes and location where avalanches are observed on pre- and post-event images.
Jupyter Notebook - 205.7 KB - MD5: 925fa20e4a267e6bbde2df7d76ebb27c
Jupyter Notebook to read avalanche catalogue in pickle
Plain Text - 313 B - MD5: e228576178734792c99c4c811486ff69
Requirements to create the Python environment needed for the Jupyter Notebook
Adobe PDF - 730.1 KB - MD5: 25d2639e92d8162f5a5737ca51368f44
Article figure 2 bottom panel showing post S1000a event avalanche map
ZIP Archive - 2.2 MB - MD5: e3f115c61c9fb92efc3ad61edc0273d5
ZIP Archive - 4.6 MB - MD5: 10e51714e4fc15a58d436b124fdb8f91
Feb 22, 2022
Durán, Cecilia; Khan, Amir; Ceylan, Savas; Zenhäusern, Géraldine; Stähler, Simon; Clinton, John; Giardini, Domenico, 2022, "Updated interior structure models of Mars from inversion of direct, reflected, and converted body waves", https://doi.org/10.18715/IPGP.2022.kzwpiude, IPGP Research Collection, V1
This dataset contains 1000 seismic models of Mars compatible with seismic travel times and converted seismic waves of high-quality marsquakes observed until October 2021. The employed data set and the inversion procedure are detailed in Duran et al.: Seismology on Mars: an analys...
Plain Text - 678 B - MD5: 6f7f23511090657a667a2b47ccdc2bcd
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