Coupled CFD-DEM simulations show frictional instability arises from coupled evolution of pore pressure, drainage, dilation/compaction, hydraulic connectivity, and granular fabric rather than pore pressure alone.
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Laser Ionisation Mass Spectrometry can detect organic molecules, microstructures, and sulphur isotope fractionation as signatures of life for future Solar System missions, with machine learning aiding unbiased analysis.
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Investigating frictional instability due to pressurization in granular media: insights from coupled computational fluid dynamics discrete element method
Coupled CFD-DEM simulations show frictional instability arises from coupled evolution of pore pressure, drainage, dilation/compaction, hydraulic connectivity, and granular fabric rather than pore pressure alone.
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Laser-based mass spectrometry for the detection of signatures of life within our Solar System
Laser Ionisation Mass Spectrometry can detect organic molecules, microstructures, and sulphur isotope fractionation as signatures of life for future Solar System missions, with machine learning aiding unbiased analysis.