Turbulent Flows with Multi-Physics
Wall-bounded Turbulent Flows
Vortical structures of turbulent Poiseuille flow at Reτ = 180
Transition from laminar flow to turbulent flow at Reτ = 180
Reynolds number dependency; Reτ = 180 (top), 550 (middle), 1000 (bottom)
Turbulent Convection
Rayleigh-Bènard Convection (Ra = 6e6, Pr = 1)
Reactive Turbulent Flows
Ammonia/Hydrogen/Nitrogen Combustion
(Video from APS-DFD Gallery of Fluid Motions, 2021)
(Video from APS-DFD Gallery of Fluid Motions, 2021)
Hypersonic Flows
Simulation of Apollo 13 re-entry
(Courtesy - M. Gallis, Sandia National Labs)
(Courtesy - M. Gallis, Sandia National Labs)
Kelvin-Helmholtz instability in hypersonic flows
(Left) Ma = 0.3 (Right) Ma = 3.0
(Left) Ma = 0.3 (Right) Ma = 3.0
Multi-Phase Turbulent Flows
To be updated.
Magnetohydrodynamics (MHD) Turbulent Flows
To be updated.
Data-driven Science and Engineering
Operator Regression with Physics-Informed Neural Networks
Data Reconciliation with Convolutional Neural Networks
High-Performance Computing
The benchmark result of our in-house simulation software shows great performance from a hundred processors to a million processors. Now, we are developing a new simulation software that will be efficient in state-of-the-art computing systems with heterogeneous architectures.
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