title: Magnetically Induced Rotating Rayleigh-Taylor Instability.
abstract: Classical techniques for investigating the Rayleigh-Taylor instability include using compressed gasses1, rocketry2or linear electric motors3to reverse the effective direction of gravity, and accelerate the lighter fluid toward the denser fluid. Other authorse.g.4,5,6have separated a gravitationally unstable stratification with a barrier that is removed to initiate the flow. However, the parabolic initial interface in the case of a rotating stratification imposes significant technical difficulties experimentally. We wish to be able to spin-up the stratification into solid-body rotation and only then initiate the flow in order to investigate the effects of rotation upon the Rayleigh-Taylor instability. The approach we have adopted here is to use the magnetic field of a superconducting magnet to manipulate the effective weight of the two liquids to initiate the flow. We create a gravitationally stable two-layer stratification using standard flotation techniques. The upper layer is less dense than the lower layer and so the system is Rayleigh-Taylor stable. This stratification is then spun-up until both layers are in solid-body rotation and a parabolic interface is observed. These experiments use fluids with low magnetic susceptibility, |χ| ~ 10-6- 10-5, compared to a ferrofluids. The dominant effect of the magnetic field applies a body-force to each layer changing the effective weight. The upper layer is weakly paramagnetic while the lower layer is weakly diamagnetic. When the magnetic field is applied, the lower layer is repelled from the magnet while the upper layer is attracted towards the magnet. A Rayleigh-Taylor instability is achieved with application of a high gradient magnetic field. We further observed that increasing the dynamic viscosity of the fluid in each layer, increases the length-scale of the instability.
authors.affiliation: School of Mathematical Sciences, University of Nottingham; matthew.scase@nottingham.ac.uk.
authors.forename: Matthew M
authors.initials: MM
authors.lastname: Scase
authors.affiliation: Faculty of Engineering, University of Nottingham.
authors.forename: Kyle A
authors.initials: KA
authors.lastname: Baldwin
authors.affiliation: School of Physics and Astronomy, University of Nottingham.
authors.forename: Richard J A
authors.initials: RJ
authors.lastname: Hill
mesh_terms: D003198:Computer Simulation; D008280:Magnetics; D008962:Models, Theoretical; D012212:Rheology / Q000379:methods*; D012399:Rotation; D014783:Viscosity