Abstract
Here, we propose a conceptual framework of Aeolian sediment transport initiation that includes the role of turbulence. Upon increasing the wind shear stress τ above a threshold value τ t ′ , particles resting at the bed surface begin to rock in their pockets because the largest turbulent fluctuations of the instantaneous wind velocity above its mean value u ¯ induce fluid torques that exceed resisting torques. Upon a slight further increase of τ , rocking turns into a rolling regime (i.e., rolling threshold τ t ≃ τ t ′ ) provided that the ratio between the integral time scale T i ∝ δ / u ¯ (where δ is the boundary layer thickness) and the time T e ∝ d / [ ( 1 − 1 / s ) g ] required for entrainment (where d is the particle diameter and s the particle–air–density ratio) is sufficiently large. Rolling then evolves into mean-wind-sustained saltation transport provided that the mean wind is able to compensate energy losses from particle-bed rebounds. However, when T i / T e is too small, the threshold ratio scales as τ t / τ t ′ ∝ T e / T i ∝ s d 2 / δ 2 , consistent with experiments. Because δ / d controls T i / T e and the relative amplitude of turbulent wind velocity fluctuations, we qualitatively predict that Aeolian sediment transport in natural atmospheres can be initiated under weaker (potentially much weaker) winds than in wind tunnels, consistent with indirect observational evidence on Earth and Mars.
Highlights
What is the wind shear stress (τ) required to initiate Aeolian sediment transport by atmospheric wind on Earth and other planetary bodies? The answer to this question is thought to be critical for predicting dust aerosol emission in climate models [1,2,3,4], planetary sediment transport and bedform evolution [5,6,7], and for inferring atmospheric wind conditions from sediment transport observations [8,9,10]
Equation (15) resembles the scaling (Equation (1)) that collapses most of the experimental data by Williams et al [11] because A0 is relatively constant for the experimental range of Galileo numbers (Ga ∈ (19, 554)). This constancy of A0 follows from the constancy of the saltation threshold As measured in wind tunnel experiments that mimic the atmosphere on Earth and produce a fully developed turbulent boundary layer (Figure 15a of Durán et al [46]), for which
That the density ratio s has a strong influence on the saltation initiation threshold As for a constant
Summary
What is the wind shear stress (τ) required to initiate Aeolian sediment transport by atmospheric wind on Earth and other planetary bodies? The answer to this question is thought to be critical for predicting dust aerosol emission in climate models [1,2,3,4], planetary sediment transport and bedform evolution [5,6,7], and for inferring atmospheric wind conditions from sediment transport observations [8,9,10]. We suspect that the one extreme outlier for d = 165 μm may either have been a faulty measurement or be associated with the observation that the boundary layer for this particular sand sample was not always fully turbulent [11] This scaling is very unusual as it fundamentally differs from the currently well-established point of view [14,15] that, for cohesionless sediments, A is only a function p of s and the particle Reynolds number. We test the predictions of our framework with existing and new threshold measurements that have been carried out for varying density ratio s, Galileo number Ga , and boundary layer thickness δ (Section 3), and discuss the potential threshold dependency on s for a constant Ga (Section 3). This dependency is quite controversial [14,15,34], and we suggest that it may be an artifact of a strongly varying thickness δ of the boundary layers produced by the different experimental facilities
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