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20112026
most citedTurbulent superstructures in Rayleigh-Bénard convection

203 citations · 1k across the 30 of their papers we have counts for

collaborators

30 papers

physics.flu-dyn2026

Thermal convection in one, two, three and four dimensions

Ambrish Pandey, Harshit Tiwari, Katepalli R. Sreenivasan

We study by means of direct numerical simulations the influence of the dimensionality of convection on flow properties. We call attention to a few general principles from consideri…

physics.flu-dyn2026★ 1 cited

Influence of plume activity on thermal convection in a rectangular cell

Ambrish Pandey, Jörg Schumacher, Matteo Parsani +1

We present three-dimensional direct numerical simulations of turbulent Rayleigh-Bénard convection in a closed rectangular box whose width and length are 0.8 and 2.4 tim…

physics.flu-dyn2025★ 1 cited

Scale-resolved turbulent Prandtl number for Rayleigh-Bénard convection at

Shashwat Bhattacharya, Dmitry Krasnov, Ambrish Pandey +2

We present a framework to calculate the scale-resolved turbulent Prandtl number for the well-mixed and highly inertial bulk of a turbulent Rayleigh-Bénard mesoscale convecti…

physics.flu-dyn2025★ 4 cited

Transient and steady convection in two dimensions

Ambrish Pandey, Katepalli R. Sreenivasan

We simulate thermal convection in a two-dimensional square box using the no-slip condition on all boundaries, and isothermal bottom and top walls and adiabatic sidewalls. We choose…

physics.flu-dyn2025★ 7 cited

Turbulent mesoscale convection in the Boussinesq limit and beyond

Shadab Alam, Dmitry Krasnov, Ambrish Pandey +4

Mesoscale convection covers an intermediate scale range between small-scale turbulence and the global organization of the convection flow. It is often characterized by an order of…

physics.flu-dyn2024★ 3 cited

Turbulent convection in rotating slender cells

Ambrish Pandey, Katepalli R. Sreenivasan

Turbulent convection in the interiors of the Sun and the Earth occurs at high Rayleigh numbers , low Prandtl numbers , and different levels of rotation rates. To understand…

physics.flu-dyn2022★ 12 cited

Similarities between characteristics of convective turbulence in confined and extended domains

Ambrish Pandey, Dmitry Krasnov, Jörg Schumacher +2

To understand turbulent convection at very high Rayleigh numbers typical of natural phenomena, computational studies in slender cells are an option if the needed resources have to…

physics.flu-dyn2022★ 28 cited

Combined particle image velocimetry and thermometry of turbulent superstructures in thermal convection

Sebastian Moller, Theo Käufer, Ambrish Pandey +2

Turbulent superstructures in horizontally extended three-dimensional Rayleigh-Bénard convection flows are investigated in controlled laboratory experiments in water at Prandtl numb…

physics.flu-dyn2022★ 27 cited

Convective mesoscale turbulence at very low Prandtl numbers

Ambrish Pandey, Dmitry Krasnov, Katepalli R. Sreenivasan +1

Horizontally extended turbulent convection, termed mesoscale convection in natural systems, remains a challenge to investigate in both experiments and simulations. This is particul…

physics.flu-dyn2021★ 14 cited

Convective heat transport in slender cells is close to that in wider cells at high Rayleigh and Prandtl numbers

Ambrish Pandey, Katepalli R. Sreenivasan

Direct numerical simulations of turbulent convection at high Rayleigh numbers in large aspect ratio cells are challenging because of the prohibitive computational resources require…

physics.flu-dyn2021★ 16 cited

Non-Boussinesq convection at low Prandtl numbers relevant to the Sun

Ambrish Pandey, Jörg Schumacher, Katepalli R. Sreenivasan

Convection in the Sun occurs at Rayleigh numbers, , as high as , molecular Prandtl numbers, , as low as , under conditions that are far from satisfying th…

physics.flu-dyn2021★ 38 cited

Thermal boundary layer structure in low-Prandtl-number turbulent convection

Ambrish Pandey

We study the structure of the thermal boundary layer (BL) in Rayleigh-Bénard convection for Prandtl number () 0.021 by conducting direct numerical simulations in a two-dimensio…

physics.flu-dyn2020★ 21 cited

Non-Boussinesq low-Prandtl number convection with a temperature-dependent thermal diffusivity

Ambrish Pandey, Jörg Schumacher, Katepalli R. Sreenivasan

In an attempt to understand the role of the strong radial dependence of thermal diffusivity on the properties of convection in sun-like stars, we mimic that effect in non-Oberbeck-…

physics.flu-dyn2019★ 12 cited

Lagrangian coherent sets in turbulent Rayleigh-Bénard convection

Christiane Schneide, Martin Stahn, Ambrish Pandey +4

Coherent circulation rolls and their relevance for the turbulent heat transfer in a two-dimensional Rayleigh--Bénard convection model are analyzed. The flow is in a closed cell of…

physics.flu-dyn2018★ 44 cited

Probing turbulent superstructures in Rayleigh-Bénard convection by Lagrangian trajectory clusters

Christiane Schneide, Ambrish Pandey, Kathrin Padberg-Gehle +1

We analyze large-scale patterns in three-dimensional turbulent convection in a horizontally extended square convection cell by Lagrangian particle trajectories calculated in direct…

physics.flu-dyn2018★ 13 cited

Transition to turbulence scaling in Rayleigh-Bénard convection

Jörg Schumacher, Ambrish Pandey, Victor Yakhot +1

If a fluid flow is driven by a weak Gaussian random force, the nonlinearity in the Navier-Stokes equations is negligibly small and the resulting velocity field obeys Gaussian stati…

physics.flu-dyn2018★ 8 cited

Reversals in infinite-Prandtl-number Rayleigh-Bénard convection

Ambrish Pandey, Mahendra K. Verma, Mustansir Barma

Using direct numerical simulations, we study the statistical properties of reversals in two-dimensional Rayleigh-Bénard convection for infinite Prandtl number. We find that the lar…

physics.flu-dyn2018★ 203 cited

Turbulent superstructures in Rayleigh-Bénard convection

Ambrish Pandey, Janet D. Scheel, Jörg Schumacher

Turbulent Rayleigh-Bénard convection displays a large-scale order in the form of rolls and cells on lengths larger than the layer height once the fluctuations of temperature and ve…

physics.flu-dyn2018★ 56 cited

Complexity of viscous dissipation in turbulent thermal convection

Shashwat Bhattacharya, Ambrish Pandey, Abhishek Kumar +1

Using direct numerical simulations of turbulent thermal convection for Rayleigh number () between and and unit Prandtl number, we derive scaling relation…

physics.flu-dyn2017★ 16 cited

On the Applicability of Low-Dimensional Models for Convective Flow Reversals at Extreme Prandtl Numbers

Manu Mannattil, Ambrish Pandey, Mahendra K. Verma +1

Constructing simpler models, either stochastic or deterministic, for exploring the phenomenon of flow reversals in fluid systems is in vogue across disciplines. Using direct numeri…

physics.flu-dyn2016★ 57 cited

Transitional boundary layers in low-Prandtl-number convection

Jörg Schumacher, Vinodh Bandaru, Ambrish Pandey +1

The boundary layer structure of the velocity and temperature fields in turbulent Rayleigh-Benard flows in closed cylindrical cells of unit aspect ratio is revisited from a transiti…

physics.flu-dyn2016★ 127 cited

Phenomenology of buoyancy-driven turbulence: recent results

Mahendra K. Verma, Abhishek Kumar, Ambrish Pandey

In this paper, we review the recent developments in the field of buoyancy-driven turbulence. Scaling and numerical arguments show that the stably-stratified turbulence with moderat…

physics.flu-dyn2016★ 24 cited

Dynamics of large-scale quantities in Rayleigh-Bénard convection

Ambrish Pandey, Abhishek Kumar, Anando G. Chatterjee +1

In this paper we estimate the relative strengths of various terms of the Rayleigh-Bénard equations. Based on these estimates and scaling analysis, we derive a general formula for t…

physics.flu-dyn2016★ 91 cited

Scaling of large-scale quantities in Rayleigh-Bénard convection

Ambrish Pandey, Mahendra K. Verma

We derive a formula for the Péclet number () by estimating the relative strengths of various terms of the momentum equation. Using direct numerical simulations in thre…