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A second-order resolvent formulation for the analysis of turbulent flow structures
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Explicit iteration of an unbounded solution of turbulent flow model involving ψ-Riemann–Liouville fractional derivatives
Published 2025-02-01Subjects: Get full text
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3
Aerodynamic Performance of Different Trailing-edge Serrations for High Reynolds Number Flows around Wing-flap System
Published 2025-02-01Subjects: Get full text
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Stable schemes for second-moment turbulent models for incompressible flows
Published 2023-09-01Subjects: Get full text
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Investigation on the influencing mechanism and quantitative evaluation of stirred heat effect in high-speed mechanical seals
Published 2025-03-01“…Secondly, in terms of heat generation, because of the high-speed shear effect of rotor, a much larger effective viscosity, radial velocity gradient, turbulence intensity and turbulence dissipation rate are generated by the turbulent flow in sealed chamber, which are responsible for the significant stirred heat. …”
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Deep reinforcement learning for active flow control in a turbulent separation bubble
Published 2025-02-01“…This allows to significantly reduce the computational cost of DRL training in a turbulent-flow environment. On the fine grid, the periodic control is able to reduce the TSB area by 6.8%, while the DRL-based control achieves 9.0% reduction. …”
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Radiatively driven convection: diffusivity-free regimes of geophysical and astrophysical flows in the laboratory
Published 2024-12-01“…The widespread belief is that the transport properties of the turbulent flow should be independent of the tiny molecular diffusivities for asymptotically strong driving, but the associated “ultimate” scaling regime proves challenging to observe experimentally using standard convection cells (Rayleigh–Bénard geometry). …”
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Uncertainties in the finite-time Lyapunov exponent in an ocean ensemble prediction model
Published 2025-02-01“…Generally, trajectory simulations, such as Lagrangian trajectories, inherit uncertainty from the underlying ocean model, bearing substantial uncertainties as a result of chaotic and turbulent flow fields. As the FTLE characterizes the flow, which may impact particle transport, we aim to investigate the uncertainty of FTLE fields at any given time using an ensemble prediction system (EPS) to propagate velocity field uncertainty into the FTLE analysis. …”
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Assessing the salinization mechanisms of coastal brackish springs
Published 2023-03-01“…To this end, we derive the equations governing variable-density turbulent flow through the conduits. These turn out to be similar to the traditional ones, except that (1) Bernouilli’s head (energy per unit weight) is substituted by the energy per unit volume, and (2) this energy is not a potential, as a flow path dependent term needs to be added. …”
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Turbulence modeling and simulation advances in CFD during the past 50 years
Published 2022-10-01“…This paper is a short retrospective review of the predictive methods of turbulent flows in Computational Fluid Dynamics over the last 50 years since the first development of computers. …”
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Experimental and Computational Fluid Dynamics: decades of turbulent EFD/CFD complementarity
Published 2022-10-01“…An overview of the parallel evolution of computations and experiments in fluid dynamics in the context of turbulent flows is given, viewed from an experimental side. …”
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CFD for turbulence: from fundamentals to geophysics and astrophysics
Published 2022-12-01“…Over the years, the combination of computational fluid dynamics (CFD) and theoretical models have critically contributed to improving our understanding of the nature of turbulent flows. In this paper, we review the role of CFD in the study of turbulence through both direct numerical simulations and the resolution of statistical multi-scale theories. …”
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Exploring the Complex Heliotail Boundary by an Extended Level Set Approach
Published 2025-01-01“…We find that the f _HP = 0 criterion, the standard heliopause definition used by other models to determine where solar wind and interstellar plasma meet, is impacted in the heliotail, where there is a broad mixing region of solar wind and interstellar medium plasma, by the nature of turbulent flows in the heliotail. We explore a different isosurface, defined by f _HP = 0.99, where the interface is composed of 99.5% solar wind and 0.50% interstellar medium. …”
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