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Seasonal variations of sub-surface seismic velocities observed by the SEIS-InSight seismometer on Mars
  • +10
  • Nicolas Compaire,
  • Ludovic Margerin,
  • Marc Monnereau,
  • Raphael F. Garcia,
  • Lange Lucas,
  • Marie Calvet,
  • Simon Staehler,
  • Nikolaj Dahmen,
  • Nils Mueller,
  • Philippe Lognonné,
  • Matthias Grott,
  • Tilman Spohn,
  • William Banerdt
Nicolas Compaire
Institut Supérieur de l'Aéronautique et de l'Espace

Corresponding Author:nicolas.compaire@isae-supaero.fr

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Ludovic Margerin
Observatory Midi-Pyrenees
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Marc Monnereau
Observatory Midi-Pyrenees
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Raphael F. Garcia
Institut Supérieur de l'Aéronautique et de l'Espace
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Lange Lucas
Laboratoire de Météorologie Dynamique/Institut Pierre Simon Laplace (LMD/IPSL), Sorbonne Université, Centre National de la Recherche Scientifique (CNRS), École Polytechnique, École Normale Supérieure (ENS), Campus Pierre et Marie Curie BC99, Paris, France
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Marie Calvet
IRAP - Universite de Toulouse
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Simon Staehler
ETH Zurich
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Nikolaj Dahmen
ETH Swiss Federal Institute of Technology Zurich
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Nils Mueller
German Aerospace Center DLR Berlin
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Philippe Lognonné
Université de Paris, Institut de physique du globe de Paris, CNRS
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Matthias Grott
German Aerospace Ctr DLR
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Tilman Spohn
German Aerospace Center DLR Berlin
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William Banerdt
JPL/NASA/Caltech
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Abstract

The SEIS seismometer deployed at the surface of Mars in the framework of the NASA-InSight mission has been continuously recording the ground motion at Elysium Planitia for more than one martian year. In this work, we investigate the seasonal variation of the near surface properties using both background vibrations and a particular class of high-frequency seismic events. We present measurements of relative velocity changes over one martian year and show that they can be modeled by a thermoelastic response of the Martian regolith. Several families of high-frequency seismic multiplets have been observed at various periods of the martian year. These events exhibit repeatable waveforms with an emergent character and a coda that is likely composed of scattered waves. Taking advantage of these properties, we use coda waves interferometry to measure relative travel-time changes as a function of the date of occurrence of the quakes. While in some families a stretching of the coda waveform is clearly observed, in other families we observe either no variation or a clear contraction of the waveform. Measurements of velocity changes from the analysis of background vibrations above 5Hz are consistent with the results from coda wave interferometry. We identify a frequency band structure in the power spectral density, that can be tracked over hundreds of days. This band structure is the equivalent in the frequency domain of an autocorrelogram and can be efficiently used to measure relative travel-time changes as a function of frequency. The observed velocity changes can be adequately modeled by the thermoelastic response of the regolith to the time-dependent incident solar flux at the seasonal scale. In particular, the model captures the time delay between the surface temperature variations and the velocity changes in the sub-surface. Our observations could serve as a basis for a joint inversion of the seismic and thermal properties in the first meters below InSIght.