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Empirical H/V spectral ratios at the InSight landing site and implications for the martian subsurface structure
- Source :
- Carrasco , S , Knapmeyer-Endrun , B , Margerin , L , Schmelzbach , C , Onodera , K , Pan , L , Lognonné , P , Menina , S , Giardini , D , Stutzmann , E , Clinton , J , Stähler , S , Schimmel , M , Golombek , M , Hobiger , M , Hallo , M , Kedar , S & Banerdt , W B 2022 , ' Empirical H/V spectral ratios at the InSight landing site and implications for the martian subsurface structure ' , Geophysical Journal International , vol. 232 , no. 2 , pp. 1293-1310 .
- Publication Year :
- 2022
-
Abstract
- The horizontal-to-vertical (H/V) spectral ratio inversion is a traditional technique for deriving the local subsurface structure on Earth. We calculated the H/V from the ambient vibrations at different wind levels at the InSight landing site, on Mars, and also computed the H/V from the S-wave coda of the martian seismic events (marsquakes). Different H/V curves were obtained for different wind periods and from the marsquakes. From the ambient vibrations, the recordings during low-wind periods are close to the instrument self-noise level. During high-wind periods, the seismic recordings are highly contaminated by the interaction of the lander with the wind and the martian ground. Therefore, these recordings are less favourable for traditional H/V analysis. Instead, the recordings of the S-wave coda of marsquakes were preferred to derive the characteristic H/V curve of this site between 0.4 and 10 Hz. The final H/V curve presents a characteristic trough at 2.4 Hz and a strong peak at 8 Hz. Using a full diffuse wavefield approach as the forward computation and the Neighbourhood Algorithm as the sampling technique, we invert for the 1-D shear wave velocity structure at the InSight landing site. Based on our inversion results, we propose a strong site effect at the InSight site to be due to the presence of a shallow high-velocity layer (SHVL) over low-velocity units. The SHVL is likely placed below a layer of coarse blocky ejecta and can be associated with Early Amazonian basaltic lava flows. The units below the SHVL have lower velocities, possibly related to a Late Hesperian or Early Amazonian epoch with a different magmatic regime and/or a greater impact rate and more extensive weathering. An extremely weak buried low velocity layer (bLVL) between these lava flows explains the data around the 2.4 Hz trough, whereas a more competent bLVL would not generate this latter feature. These subsurface models are in good agreement with results from hammering experiment and compl
Details
- Database :
- OAIster
- Journal :
- Carrasco , S , Knapmeyer-Endrun , B , Margerin , L , Schmelzbach , C , Onodera , K , Pan , L , Lognonné , P , Menina , S , Giardini , D , Stutzmann , E , Clinton , J , Stähler , S , Schimmel , M , Golombek , M , Hobiger , M , Hallo , M , Kedar , S & Banerdt , W B 2022 , ' Empirical H/V spectral ratios at the InSight landing site and implications for the martian subsurface structure ' , Geophysical Journal International , vol. 232 , no. 2 , pp. 1293-1310 .
- Notes :
- application/pdf, English
- Publication Type :
- Electronic Resource
- Accession number :
- edsoai.on1382510742
- Document Type :
- Electronic Resource