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Jaywant H. Arakeri

Publications and source records attributed to Jaywant H. Arakeri.

6 recordsLinked to original sources

Clapping propulsion and thin vortex rings: a computational study of vortex dynamics, energy equivalence, and core potential energy

We report a computational study of clapping propulsion using two thin rigid plates forming a 60-degree interplate cavity that generates a thrust-producing jet during closure. Plate kinematics are prescribed from experiments for two cases: dynamic and stationary, with forward motion constrained in the latter. The computations show that interplate pressure is higher in the stationary case compared to that in the dynamic case, resulting in differences in the thrust produced and in the evolution of wake vortices, with the stationary case forming triangular and Omega-shaped loops, while the dynamic case forms an elliptical loop for each plate. We examine the energy budget in the post-clapping phase, when the vortices are fully formed. The energy consists of kinetic energy and a component associated with vortex formation, whose sum approximately matches the work done on the fluid. This extra term, which we call the core potential energy, is found to be equal to the integral of pressure over the core volume of the vortex. This component is also checked using separate axisymmetric vortex ring simulations, where the kinetic energy is about 60% of the injected slug energy, and the remaining part is the core potential energy. Sullivan et al.(2008) had commented on this deficit for vortex rings and hypothesized the existence of a potential energy associated with the vortex structure.

physics.flu-dyn↗

The role of viscosity contrast on plume structure in laboratory modeling of mantle convection

We have conducted laboratory experiments to model important aspects of plumes in mantle convection. We focus on the role of the viscosity ratio U (between the ambient fluid and the plume fluid) in determining the plume structure and dynamics. In our experiments, we are able to capture geophysical convection regimes relevant to mantle convection both for hot spots (when U > 1) and plate-subduction (when U < 1) regimes. The planar laser induced fluorescence (PLIF) technique is used for flow visualization and characterizing the plume structures. The convection is driven by compositional buoyancy generated by the perfusion of lighter fluid across a permeable mesh and the viscosity ratio U is systematically varied over a range from 1/300 to 2500. The planform, near the bottom boundary for U=1, exhibits a well-known dendritic line plume structure. As the value of U is increased, a progressive morphological transition is observed from the dendritic-plume structure to discrete spherical plumes, accompanied with thickening of the plumes and an increase in the plume spacing. In the vertical section, mushroom-shaped plume heads at U=1 change into intermittent spherical-blob shaped plumes at high U, resembling mantle plume hot spots in mantle convection. In contrast, for low values of U (~1/300), the regime corresponds to subduction of plates in the mantle. In this regime, we observe for the first time that plumes arise from a thick boundary with cellular structure and develop into sheet-plumes. We use experimental data to quantify these morphological changes and mixing dynamics of the plumes at different regimes of U. We also compare our observations on plume spacing with various models reported in the literature by varying the viscosity ratio and the buoyancy flux.

physics.flu-dyn↗

A Pitching Foil with a Flexible flap Creates an Orderly Jet

We experimentally studied the effect of flexibility on the flow produced by sinusoidally pitching foil in quiescent fluid. The rigid foil produces a weak, divergent and meandering jet. On the contrary, the foil with a flexible flap produces an orderly, narrow, coherent jet. It has been observed that such orderly jet is produced when the flap has appropriate flexibility. The jet produced in quiescent fluid by the flexible foil is accompanied by a corresponding thrust. In that sense, this is simple and different type of hovering.

physics.flu-dyn↗

Multifractal nature of plume structure in high Rayleigh number convection

The geometrically different plan forms of near wall plume structure in turbulent natural convection, visualised by driving the convection using concentration differences across a membrane, are shown to have a common multifractal spectrum of singularities for Rayleigh numbers in the range $10^{10}- 10^{11}$ at Schmidt number of 602. The scaling is seen for a length scale range of $2^5$ and is independent of the Rayleigh number, the flux, the strength and nature of the large scale flow, and the aspect ratio. Similar scaling is observed for the plume structures obtained in the presence of a weak flow across the membrane. This common non trivial spatial scaling is proposed to be due to the same underlying generating process of the near wall plume structures.

nlin.PS↗

Flux scaling and plume structure in high Ra - high Sc turbulent convection

The arrangement of brine above water across a micro porous permeable membrane is used to study high Rayleigh Number($10^{11}- 10^{10}$) high Schmidt number(650)turbulent convection. The flux shows 4/3$^{rd}$ scaling with line plume as the near wall coherent structures. Shifting of multiple large scale flow cells result in changing near membrane mean shear directions for large aspect ratios. Lower aspect ratios show single large scale flow cell and constant sense of mean shear.

physics.flu-dyn↗

Integral analysis of laminar indirect free convection boundary layers with weak blowing for Schmidt no. ~ 1

Laminar natural convection at unity Schmidt number over a horizontal surface with a weak normal velocity at the wall is studied using an integral analysis. To characterise the strength of the blowing, we define a non-dimensional parameter called the blowing parameter. After benchmarking with the no blowing case, the effect of the blowing parameter on boundary layer thickness, velocity and concentration profiles is obtained. Weak blowing is seen to increase the wall shear stress. For blowing parameters greater than unity, the diffusional flux at the wall becomes negligible and the flux is almost entirely due to the blowing.

physics.flu-dyn↗