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- W2143661982 abstract "Dunes and bedforms are observed in considerably diverse environments: aeolian dunes of sand as well as snow, dunes under water, but also dunes on Mars or Titan. Summarising our work published in [1], we would like to show in this paper that, although the fluid, the grains and the mode of sediment transport can be different in these various situations, the understanding of the size at which a flat bed destabilises – denoted below as the ‘elementary’ size – can be thought of in a common manner, i.e. independently of the above geological objects. Reasoning in terms of instability mechanism, we have then been able to evidence a scaling law for this elementary size, valid from centimetric subaqueous ripples to 600 m long Martian dunes." @default.
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- W2143661982 date "2008-01-01" @default.
- W2143661982 modified "2023-09-27" @default.
- W2143661982 title "Dunes on Mars, 'Venus', Earth, and Subaqueous Ripples: A Scaling Law for Their Elementary Size" @default.
- W2143661982 hasPublicationYear "2008" @default.
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