Turbulent Transport Processes at Rough Surfaces with Geophysical Applications

Procedia IUTAM Elsevier 15 (2015) 34-40

Authors:

Srikanth Toppaladoddi, Sauro Succi, John S Wettlaufer

Slender axisymmetric Stokesian swimmers

Journal of Fluid Mechanics Cambridge University Press (CUP) 746 (2014) 273-299

Authors:

S Toppaladoddi, NJ Balmforth

Steady turbulent density currents on a slope in a rotating fluid

Journal of Fluid Mechanics Cambridge University Press (CUP) 746 (2014) 405-436

Authors:

GE Manucharyan, W Moon, F Sévellec, AJ Wells, J-Q Zhong, JS Wettlaufer

Nonlinear mushy-layer convection with chimneys: stability and optimal solute fluxes

JOURNAL OF FLUID MECHANICS 716 (2013) 203-227

Authors:

Andrew J Wells, JS Wettlaufer, Steven A Orszag

Mushy-layer dynamics in micro and hyper gravity

Physics of Fluids 24:10 (2012)

Authors:

JG O'Rourke, AJE Riggs, CA Guertler, PW Miller, CM Padhi, MM Popelka, AJ Wells, AC West, JQ Zhong, JS Wettlaufer

Abstract:

We describe the results of experiments on mushy layers grown from aqueous ammonium chloride solution in normal, micro, and hyper gravity environments. In the fully developed chimney state, the chimney plume dynamics differ strikingly when conditions change from micro to hyper gravity. In microgravity, we find fully arrested plume motion and suppressed convection. As gravity exceeds Earth conditions, we observe a host of phenomena, ranging from arched plumes that undergo forced Rayleigh-Taylor instabilities to in-phase multiple plume oscillatory behavior. For the same initial solute concentrations and fixed boundary cooling temperatures, we find that, in runs of over two hours, the averaged effects of microgravity and hypergravity result in suppressed growth of the mushy layers, a phenomenon caused by a net enhancement of convective heat and solute transport from the liquid to the mushy layers. These behaviors are placed in the context of the theory of convecting mushy layers as studied under normal laboratory conditions. © 2012 American Institute of Physics.