Abstract
Ripples are ubiquitous on Earth and other planets and can act as
valuable (paleo) environmental indicators of terrestrial and
extraterrestrial sedimentary landscapes. Recently, Lapotre et al.
established an empirical relationship that describes current ripple
wavelengths and indicates a dependence on bed shear stresses. However,
the fluid mechanics controlling ripple wavelengths are still poorly
understood, and empirical relationships cannot be easily applied to
extraterrestrial landscapes. We used numerical modeling to investigate
the physics linking flow conditions to current ripple morphology and
spacing. Our analysis used large eddy simulations based on a
Lattice-Boltzmann numerical flow model. Results showed that shear
velocities varied spatially depending on ripple separation, with largest
stresses found between separation bubbles and downstream crests. We
further considered differences in the sum of non-dimensional bed-load
fluxes caused by positive (downstream directed) and negative (upstream
directed) shear stresses at ripple crest. Preliminary analyses indicate
that modeling results were closer to the empirical relationship as
differences in bed-load fluxes at ripple crest decreased. This
observation might suggest that the empirical relationship linking ripple
wavelengths and bed shear stresses represents sediment transport
conditions at ripple crests, possibly a minimum in net bed-load fluxes.
Original language | English |
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Publication status | Published - 1 Dec 2018 |
Keywords
- 6207 Comparative planetology
- PLANETARY SCIENCES: SOLAR SYSTEM OBJECTSDE: 5415 Erosion and weathering
- PLANETARY SCIENCES: SOLID SURFACE PLANETSDE: 5419 Hydrology and fluvial processes
- PLANETARY SCIENCES: SOLID SURFACE PLANETSDE: 5499 General or miscellaneous
- PLANETARY SCIENCES: SOLID SURFACE PLANETS