[图书][B] Physics of buoyant flows: from instabilities to turbulence

MK Verma - 2018 - World Scientific
Hydrodynamic flows exhibit turbulent behaviour which is not well understood till date. When
a fluid is in a gravitational field, the flow becomes even more complex due to the gravity …

Effects of Prandtl number in quasi-two-dimensional Rayleigh–Bénard convection

XM Li, JD He, Y Tian, P Hao, SD Huang - Journal of Fluid Mechanics, 2021 - cambridge.org
We report an experimental study of the Prandtl-number effects in quasi-two-dimensional
(quasi-2-D) Rayleigh–Bénard convection. The experiments were conducted in four …

Steady Rayleigh–Bénard convection between stress-free boundaries

B Wen, D Goluskin, M LeDuc, GP Chini… - Journal of Fluid …, 2020 - cambridge.org
Steady Rayleigh–Bénard convection between stress-free boundaries Page 1 J. Fluid Mech.
(2020), vol. 905, R4, doi:10.1017/jfm.2020.812 Steady Rayleigh–Bénard convection between …

Scaling of large-scale quantities in Rayleigh-Bénard convection

A Pandey, MK Verma - Physics of Fluids, 2016 - pubs.aip.org
We derive a formula for the Péclet number (Pe) by estimating the relative strengths of
various terms of the momentum equation. Using direct numerical simulations in three …

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

A Pandey - Journal of Fluid Mechanics, 2021 - cambridge.org
Thermal boundary layer structure in low-Prandtl-number turbulent convection Page 1 J. Fluid
Mech. (2021), vol. 910, A13. © The Author(s), 2021. Published by Cambridge University Press …

Prandtl number dependence of the small-scale properties in turbulent Rayleigh-Bénard convection

S Bhattacharya, MK Verma, R Samtaney - Physical Review Fluids, 2021 - APS
We analyze the Prandtl number (Pr) dependence of spectra and fluxes of kinetic energy, as
well as the energy injection rates and dissipation rates, of turbulent thermal convection using …

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

A Pandey, J Schumacher, KR Sreenivasan - Physical Review Fluids, 2021 - APS
Convection in the Sun occurs at Rayleigh numbers, Ra, as high as 10 22 and molecular
Prandtl numbers, Pr, as low as 10− 6, under conditions that are far from satisfying the …

Influence of Prandtl number in turbulent Rayleigh-Bénard convection over rough surfaces

M Sharma, K Chand, AK De - Physical Review Fluids, 2022 - APS
The present study numerically investigates the effect of the Prandtl number (0.1≤ Pr≤ 100)
on the flow structures and heat transport mechanism in a two-dimensional rectangular rough …

Numerical studies on the dynamics of two-layer Rayleigh-Bénard convection with an infinite Prandtl number and large viscosity contrasts

M Yoshida, Y Hamano - Physics of Fluids, 2016 - pubs.aip.org
The fundamental physics and dynamics relating to two-layer convection with an infinite
Prandtl number and large viscosity contrasts have not yet been quantitatively resolved by …

On the applicability of low-dimensional models for convective flow reversals at extreme Prandtl numbers

M Mannattil, A Pandey, MK Verma… - The European Physical …, 2017 - Springer
Constructing simpler models, either stochastic or deterministic, for exploring the
phenomenon of flow reversals in fluid systems is in vogue across disciplines. Using direct …