International audience• Rayleigh and Love waves were detected on Mars; • Seismic wave speed is directionally dependent over large-scales within Mars crust; • The shear wave horizontal velocity is faster than the vertical velocity at 10-25 km depth in the lowlands between the event and the lander
1981), and at sub-crustal depths anisotropy is likely caused by arises above ~250 km. This has been ...
Abstract. Long-period surface waves are used to map lateral heterogenefties of velocity and anisotro...
International audienceWe present global and regional synthetic seismograms computed for 1D and 3D Ma...
Abstract: The largest seismic event ever recorded on Mars, with a moment magnitude of 4.7 ±&nb...
The largest seismic event ever recorded on Mars, with a moment magnitude of 4.7 ± 0.2, is the first ...
International audienceWe analyzed broadband and low-frequency events recorded on Mars and made the f...
We detected surface waves from two meteorite impacts on Mars. By measuring group velocity dispersion...
International audienceWe detected surface waves from two meteorite impacts on Mars. By measuring gro...
Surface waves had not been observed on any marsquake records during the first 3 years of seismic mon...
We have observed both minor-arc (R1) and major-arc (R2) Rayleigh waves for the largest marsquake (ma...
We report observations of Rayleigh waves that orbit around Mars up to three times following the S122...
International audienceFor the first time, we measured the ellipticity of direct Rayleigh waves at in...
International audienceRecordings in western Tibet of Rayleigh and Love waves at periods less than 70...
[1] The sensitivity of a surface wave to the lateral structure of the Earth's mantle depends on the ...
After more than 4 Earth years of operation on the martian surface monitoring the planet’s ground vib...
1981), and at sub-crustal depths anisotropy is likely caused by arises above ~250 km. This has been ...
Abstract. Long-period surface waves are used to map lateral heterogenefties of velocity and anisotro...
International audienceWe present global and regional synthetic seismograms computed for 1D and 3D Ma...
Abstract: The largest seismic event ever recorded on Mars, with a moment magnitude of 4.7 ±&nb...
The largest seismic event ever recorded on Mars, with a moment magnitude of 4.7 ± 0.2, is the first ...
International audienceWe analyzed broadband and low-frequency events recorded on Mars and made the f...
We detected surface waves from two meteorite impacts on Mars. By measuring group velocity dispersion...
International audienceWe detected surface waves from two meteorite impacts on Mars. By measuring gro...
Surface waves had not been observed on any marsquake records during the first 3 years of seismic mon...
We have observed both minor-arc (R1) and major-arc (R2) Rayleigh waves for the largest marsquake (ma...
We report observations of Rayleigh waves that orbit around Mars up to three times following the S122...
International audienceFor the first time, we measured the ellipticity of direct Rayleigh waves at in...
International audienceRecordings in western Tibet of Rayleigh and Love waves at periods less than 70...
[1] The sensitivity of a surface wave to the lateral structure of the Earth's mantle depends on the ...
After more than 4 Earth years of operation on the martian surface monitoring the planet’s ground vib...
1981), and at sub-crustal depths anisotropy is likely caused by arises above ~250 km. This has been ...
Abstract. Long-period surface waves are used to map lateral heterogenefties of velocity and anisotro...
International audienceWe present global and regional synthetic seismograms computed for 1D and 3D Ma...
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