Acoustic Emissions of Nearly Steady and Uniform Granular Flows: A Proxy for Flow Dynamics and Velocity Fluctuations

Author:

Bachelet V.1,Mangeney A.1ORCID,Toussaint R.23ORCID,de Rosny J.4,Arran M. I.15ORCID,Farin M.4ORCID,Hibert C.2ORCID

Affiliation:

1. Université Paris Cité Institut de Physique du Globe de Paris CNRS Paris France

2. University of Strasbourg CNRS Institut Terre et Environnement de Strasbourg UMR 7063 Strasbourg France

3. PoreLab Njord Centre Department of Physics University of Oslo Oslo Norway

4. Institut Langevin ESPCI Paris Université PSL CNRS Paris France

5. LSRI Campion Hall University of Oxford Oxford UK

Abstract

AbstractThe seismic waves emitted during granular flows are generated by different sources: high frequencies by interparticle collisions and low frequencies by global motion and large scale deformation. To unravel these different mechanisms, an experimental study has been performed on the seismic waves emitted by dry, dense, quasi‐steady granular flows. The emitted seismic waves were recorded using shock accelerometers and the flow dynamics were captured with a fast camera. The mechanical characteristics of the particle collisions were analyzed, along with the intervals between collisions and the correlations in particles' motion. The high‐frequency seismic waves (1–50 kHz) were found to originate from particle collisions and waves trapped in the flowing layer. The low‐frequency waves (20–60 Hz) were generated by particles' oscillations along their trajectories, that is, from cycles of dilation/compression during coherent shear. The profiles of granular temperature (i.e., the mean squared value of particle velocity fluctuations) and average velocity were measured and related to each other, then used in a simple steady granular flow model, in which the seismic signal consists of the variously attenuated contributions of shear‐induced Hertzian collisions throughout the flow, to predict the rate at which seismic energy was emitted. Agreement with the measured seismic power was reasonable, and scaling laws relating the seismic power, the shear strain rate and the inertial number were derived. In particular, the emitted seismic power was observed to be approximately proportional to the root mean square velocity fluctuation to the power 3.1 ± 0.9, with the latter related to the mean flow velocity.

Funder

H2020 European Research Council

Institut national des sciences de l'Univers

Institut de physique

Publisher

American Geophysical Union (AGU)

Subject

Earth-Surface Processes,Geophysics

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