A systematic experimental study of rapidly rotating spherical convection in water and liquid gallium

By Julien Aubert, D. Brito, H. Nataf, P. Cardin, J. Masson. 2001

147 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology, Oceanography

View Paper: https://www.semanticscholar.org/paper/d9b02cad0aa71c142da340121dbaaf8e486fa89d

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Citations in the corpus

Zonal flow driven by strongly supercritical convection in rotating spherical shells (2002, methodology): “Effect of Prandtl number The numerical work by Zhang (1992) and the experimental results by Aubert et al. (2001) strongly suggested that the value of the Prandtl number plays an important role in the presence of a strong zonal flow.”
Sulfur's impact on core evolution and magnetic field generation on Ganymede (2005, unknown): “Using the results of recent laboratory and numerical experiments [Aubert et al., 2001; Aurnou et al., 2003; Aubert, 2005] and those presented here we can make simple estimates of the Rossby number, Ro (the ratio of inertial to Coriolis forces [Tritton, 1988]), and the magnetic Reynolds parameter,…”
The magnetic structure of convection-driven numerical dynamos (2008, background): “The inertial scaling for flow velocity in rotating convection and numerical dynamos (Aubert et al. 2001; Christensen & Aubert 2006) invokes an equilibrium between the curled inertia ∇ × ((u · ∇)u) and curled Coriolis force ∇ × (2 ez × u).”
Scaling regimes in spherical shell rotating convection (2016, methodology): “A sizeable fraction of the dissipation occurs in the fluid bulk, which is dominated by a triple force balance between Coriolis, Inertia and buoyancy (the so-called inertial theory of rotating convection or CIA balance, e.g. Aubert et al. 2001).”
Quasi-geostrophic flows responsible for the secular variation of the Earth's magnetic field (2008, background): “Columnar flows aligned with the rotation axis, z, have often been seen to emerge in laboratory experiments, as preferred self-organized structures (e.g. Cardin & Olson (1994), Aubert et al. (2001), Gillet et al. (2007) ).”
Scaling properties of convection-driven dynamos in rotating spherical shells and application to planetary magnetic fields (2006, background): “For non-magnetic convection, Aubert et al. (2001) proposed that δ z/D remains of order one due to the geostrophy of the convective flow, and that δϕ is determined by a balance between inertia and Coriolis force and increases with the vigour of convection.”
Paleomagnetic Records of Meteorites and Early Planetesimal Differentiation (2010, background): “(ii) UCIA: This velocity estimate comes from a balance of the non-geostrophic components of the Coriolis, non-linear inertial, and Archimedean (CIA) forces (Aubert et al. 2001; Christensen and Aubert 2006).”
Dynamo Scaling Laws and Applications to the Planets (2010, background): “Aubert et al. (2001) considered a balance between these three terms in the vorticity equation (CIAbalance from Coriolis, Inertia, Archimedean).”