Nan-Sheng Liu
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Nan-Sheng Liu has a total of 101 co-authors. Here are the top co-authors by number of shared publications:
- Xi-Yun Lu
University of Science and Technology of China
47 shared publications - Zhen-Hua Wan
University of Science and Technology of China
20 shared publications - Bamin Khomami
University of Tennessee
14 shared publications - Fenghui Lin
University of Science and Technology of China
13 shared publications - Zhiye Zhao
Hong Kong University of Science and Technology
13 shared publications - Peng-Jun-Yi Zhang
State Key Laboratory of High Temperature Gas Dynamics, School of Engineering Science, University of Science and Technology of China
11 shared publications
Latest Publications
- 1 August 2026
- Published by AIP Publishing in Physics of Fluids
- Vol. 38 (8)
Characteristics of the three-dimensional boundary layer over a lifting body at Mach 12
Direct numerical simulation is performed to investigate the three-dimensional turbulent boundary layer on the leeward side of the Hypersonic Transition Research Vehicle at Mach 12 and a 6° angle of attack. Under the combined influence of bypass transition induced by blowing/suction and three-dimensional effects, two spatially separated regions of enhanced skin friction and wall heat flux (WHF) are identified, denoted as regions A and B, whose formation mechanisms are fundamentally distinct. In region A, the high WHF is predominantly driven by steepened gradients induced by pressure gradients, whereas the enhanced skin friction is further driven by the unsteady separation and reattachment resulting from an adverse-to-favorable pressure gradient transition, exhibiting banded quasi-streamwise high-momentum flows. Region B, in contrast, is governed by the roll-up and breakdown of quasi-streamwise vortices, which sustain a fully developed turbulent state populated by fine-scale transverse vortical structures and azimuthally distributed heat-flux streaks. Compressibility effects are pronounced in both regions, as evidenced by the emergence of shocklets extending into the outer boundary layer. The two regions further exhibit contrasting turbulence signatures: large-scale structures driven by blowing/suction generate outer peaks in the Reynolds stresses upstream, whereas intense turbulence production in region B gives rise to distinct inner peaks. These findings highlight the critical role of geometric three-dimensionality and compressibility-induced structural changes in shaping the aerodynamic and aerothermal environment of high-speed lifting-body configurations.
- 1 August 2026
- Published by AIP Publishing in Physics of Fluids
- Vol. 38 (8)
Characteristics of the three-dimensional boundary layer over a lifting body at Mach 12
Direct numerical simulation is performed to investigate the three-dimensional turbulent boundary layer on the leeward side of the Hypersonic Transition Research Vehicle at Mach 12 and a 6° angle of attack. Under the combined influence of bypass transition induced by blowing/suction and three-dimensional effects, two spatially separated regions of enhanced skin friction and wall heat flux (WHF) are identified, denoted as regions A and B, whose formation mechanisms are fundamentally distinct. In region A, the high WHF is predominantly driven by steepened gradients induced by pressure gradients, whereas the enhanced skin friction is further driven by the unsteady separation and reattachment resulting from an adverse-to-favorable pressure gradient transition, exhibiting banded quasi-streamwise high-momentum flows. Region B, in contrast, is governed by the roll-up and breakdown of quasi-streamwise vortices, which sustain a fully developed turbulent state populated by fine-scale transverse vortical structures and azimuthally distributed heat-flux streaks. Compressibility effects are pronounced in both regions, as evidenced by the emergence of shocklets extending into the outer boundary layer. The two regions further exhibit contrasting turbulence signatures: large-scale structures driven by blowing/suction generate outer peaks in the Reynolds stresses upstream, whereas intense turbulence production in region B gives rise to distinct inner peaks. These findings highlight the critical role of geometric three-dimensionality and compressibility-induced structural changes in shaping the aerodynamic and aerothermal environment of high-speed lifting-body configurations.
- Open Access
- 18 June 2026
- Published by Cambridge University Press (CUP) in Journal of Fluid Mechanics
- Vol. 1037, A39
Dynamic interactions between a self-propelled flexible plate and multiple wall-mounted compliant blades
A numerical study is conducted on a self-propelled flexible plate moving above an array of wall-mounted compliant blades at Reynolds numbers of order 100, designed to mimic flatfish-like locomotion near the vegetation-covered seabed. Compared with a flat rigid wall located at the same vertical distance from the plate, the blade-covered wall enhances the propulsive performance of the plate, yielding a higher propulsive velocity and lower energy consumption per transport distance. This enhancement intensifies as the blade spacing and vertical distance between the plate and the bottom wall decrease, but diminishes when the flapping frequency approaches the natural frequency of the blades due to resonance. By accounting for the asymmetric motion of the plate during the upper and lower half-periods, a universal scaling law italic Re Subscript c Baseline tilde left parenthesis italic Re Subscript f comma delta Baseline right parenthesis Superscript 3 divided by 2 ${\textit{Re}}_c\sim ({\textit{Re}}_{f,\delta })^{3/2}$ is identified between the propulsive Reynolds number italic Re Subscript c ${\textit{Re}}_c$ and the corrected flapping Reynolds number italic Re Subscript f comma delta ${\textit{Re}}_{f,\delta }$ . Under the excitation of the flapping plate, two distinct vibration patterns are identified for the blade array. The first is the flapping-driven mode, which propagates synchronously with the plate’s motion. The second exhibits forward-propagating travelling waves, which are generated by the cooperative underdamped vibrations of downstream blades, and have a phase velocity much faster than the propulsive velocity of the plate. This study may shed light on the design of bio-inspired underwater vehicles and flow sensing techniques.- 18 June 2026
- Published by Cambridge University Press (CUP) in Journal of Fluid Mechanics
- Vol. 1037, A39
Open AccessDynamic interactions between a self-propelled flexible plate and multiple wall-mounted compliant blades
A numerical study is conducted on a self-propelled flexible plate moving above an array of wall-mounted compliant blades at Reynolds numbers of order 100, designed to mimic flatfish-like locomotion near the vegetation-covered seabed. Compared with a flat rigid wall located at the same vertical distance from the plate, the blade-covered wall enhances the propulsive performance of the plate, yielding a higher propulsive velocity and lower energy consumption per transport distance. This enhancement intensifies as the blade spacing and vertical distance between the plate and the bottom wall decrease, but diminishes when the flapping frequency approaches the natural frequency of the blades due to resonance. By accounting for the asymmetric motion of the plate during the upper and lower half-periods, a universal scaling law italic Re Subscript c Baseline tilde left parenthesis italic Re Subscript f comma delta Baseline right parenthesis Superscript 3 divided by 2 ${\textit{Re}}_c\sim ({\textit{Re}}_{f,\delta })^{3/2}$ is identified between the propulsive Reynolds number italic Re Subscript c ${\textit{Re}}_c$ and the corrected flapping Reynolds number italic Re Subscript f comma delta ${\textit{Re}}_{f,\delta }$ . Under the excitation of the flapping plate, two distinct vibration patterns are identified for the blade array. The first is the flapping-driven mode, which propagates synchronously with the plate’s motion. The second exhibits forward-propagating travelling waves, which are generated by the cooperative underdamped vibrations of downstream blades, and have a phase velocity much faster than the propulsive velocity of the plate. This study may shed light on the design of bio-inspired underwater vehicles and flow sensing techniques. - 10 June 2026
- Published by American Physical Society (APS) in Physical Review Fluids
- Vol. 11 (8)
Super-resolution reconstruction of nonlinear evolution of multimode Rayleigh-Taylor mixing
- 10 June 2026
- Published by American Physical Society (APS) in Physical Review Fluids
- Vol. 11 (8)
Super-resolution reconstruction of nonlinear evolution of multimode Rayleigh-Taylor mixing
- 1 June 2026
- Published by AIP Publishing in Physics of Fluids
- Vol. 38 (6)
Large-scale separation-induced secondary turbulence amplification in shock wave/turbulent boundary layer interaction
Turbulence amplification in shock wave/turbulent boundary layer interactions critically affects flow unsteadiness and wall loading in supersonic aerodynamic configurations. Direct numerical simulations (DNS) are performed at shock generator angles of β=8°, 10°, and 12°. At the two smaller angles, turbulence amplification is confined to the vicinity of the separation point. As β increases to 12°, however, a pronounced secondary amplification emerges near the reattachment point, giving rise to a bimodal streamwise distribution of turbulent kinetic energy (TKE). Spectral analysis of the TKE production terms reveals that this secondary amplification is predominantly driven by shear production associated with large-scale vortical structures. Global stability analysis (GSA) of the mean flow further demonstrates that all unstable eigenmodes are intrinsically tied to the separation bubble, and the most unstable spanwise wavenumber predicted by GSA agrees closely with the dominant scale observed in the DNS. Reduced-order variational mode decomposition identifies an energetically dominant, low-frequency three-dimensional mode in the reattachment region for the β=12° case, characterized by coherent Görtler-like vortices whose spanwise wavelength is consistent with both the DNS and GSA results. These results suggest that the secondary turbulence amplification originates from the modal instability of the mean flow associated with the large-scale separation bubble and the coherent structures it induces.
- 1 June 2026
- Published by AIP Publishing in Physics of Fluids
- Vol. 38 (6)
Large-scale separation-induced secondary turbulence amplification in shock wave/turbulent boundary layer interaction
Turbulence amplification in shock wave/turbulent boundary layer interactions critically affects flow unsteadiness and wall loading in supersonic aerodynamic configurations. Direct numerical simulations (DNS) are performed at shock generator angles of β=8°, 10°, and 12°. At the two smaller angles, turbulence amplification is confined to the vicinity of the separation point. As β increases to 12°, however, a pronounced secondary amplification emerges near the reattachment point, giving rise to a bimodal streamwise distribution of turbulent kinetic energy (TKE). Spectral analysis of the TKE production terms reveals that this secondary amplification is predominantly driven by shear production associated with large-scale vortical structures. Global stability analysis (GSA) of the mean flow further demonstrates that all unstable eigenmodes are intrinsically tied to the separation bubble, and the most unstable spanwise wavenumber predicted by GSA agrees closely with the dominant scale observed in the DNS. Reduced-order variational mode decomposition identifies an energetically dominant, low-frequency three-dimensional mode in the reattachment region for the β=12° case, characterized by coherent Görtler-like vortices whose spanwise wavelength is consistent with both the DNS and GSA results. These results suggest that the secondary turbulence amplification originates from the modal instability of the mean flow associated with the large-scale separation bubble and the coherent structures it induces.
- 26 May 2026
- Published by American Physical Society (APS) in Physical Review Fluids
- Vol. 11 (5)
Effects of interparticle collisions on turbulence modulation in particle-laden channel flow
- 26 May 2026
- Published by American Physical Society (APS) in Physical Review Fluids
- Vol. 11 (5)
Effects of interparticle collisions on turbulence modulation in particle-laden channel flow
- 25 May 2026
- Published by Cambridge University Press (CUP) in Journal of Fluid Mechanics
- Vol. 1035, A40
Polymer-induced flow transitions in turbulent Taylor–Couette flow with co- and counter-rotating cylinders
Direct numerical simulations are performed to elucidate the influence of counter- and co-rotation on turbulent viscoelastic Taylor–Couette flow in the Rossby number range $ \textit{Ro}^{-1}=-0.6$ to $ \textit{Ro}^{-1}=1$ . A novel polymer-induced transition pathway is discovered that is fundamentally different from Newtonian flows. In the counter-rotation regime, the neutral surface is elastically modified and separates the turbulent inner-wall region containing chaotic vortices from the relaminarised layer adjacent to the outer cylinder. Strikingly, co-rotation triggers an elasto-rotational instability, which leads to the breakdown of large-scale Taylor vortices into small-scale penetrating structures, thereby preventing the relaminarisation at high co-rotation rates. Examination of turbulence dynamics demonstrates that the structural changes with increasing $ \textit{Ro}^{-1}$ are accompanied by a transition from elasto-inertial to elastically dominated turbulence. Specifically, the polymer stress progressively exceeds the Reynolds stress and monotonically enhances angular momentum transport, which eliminates the optimal transport characteristic found in the Newtonian flow. The elastically dominated nature of the turbulent flow under co-rotation is further corroborated by the more significant elastic production of the turbulent kinetic energy, as well as the monotonic enhancement of the polymer elongation as $ \textit{Ro}^{-1}$ increases. Furthermore, it is indicated that the polymer orientation strongly depends on vortical structures, with enhanced radial alignment occurring in the boundary region between adjacent vortices. This vortex-mediated polymer orientation is crucial for generating substantial polymer shear stress, establishing a direct link between coherent structures and polymer dynamics.- 25 May 2026
- Published by Cambridge University Press (CUP) in Journal of Fluid Mechanics
- Vol. 1035, A40
Polymer-induced flow transitions in turbulent Taylor–Couette flow with co- and counter-rotating cylinders
Direct numerical simulations are performed to elucidate the influence of counter- and co-rotation on turbulent viscoelastic Taylor–Couette flow in the Rossby number range $ \textit{Ro}^{-1}=-0.6$ to $ \textit{Ro}^{-1}=1$ . A novel polymer-induced transition pathway is discovered that is fundamentally different from Newtonian flows. In the counter-rotation regime, the neutral surface is elastically modified and separates the turbulent inner-wall region containing chaotic vortices from the relaminarised layer adjacent to the outer cylinder. Strikingly, co-rotation triggers an elasto-rotational instability, which leads to the breakdown of large-scale Taylor vortices into small-scale penetrating structures, thereby preventing the relaminarisation at high co-rotation rates. Examination of turbulence dynamics demonstrates that the structural changes with increasing $ \textit{Ro}^{-1}$ are accompanied by a transition from elasto-inertial to elastically dominated turbulence. Specifically, the polymer stress progressively exceeds the Reynolds stress and monotonically enhances angular momentum transport, which eliminates the optimal transport characteristic found in the Newtonian flow. The elastically dominated nature of the turbulent flow under co-rotation is further corroborated by the more significant elastic production of the turbulent kinetic energy, as well as the monotonic enhancement of the polymer elongation as $ \textit{Ro}^{-1}$ increases. Furthermore, it is indicated that the polymer orientation strongly depends on vortical structures, with enhanced radial alignment occurring in the boundary region between adjacent vortices. This vortex-mediated polymer orientation is crucial for generating substantial polymer shear stress, establishing a direct link between coherent structures and polymer dynamics.- Open Access
- 4 May 2026
- Published by Cambridge University Press (CUP) in Journal of Fluid Mechanics
- Vol. 1034
Prediction of the drag, lift and torque coefficients of non-spherical particles constrained by wall
Accurate prediction of the hydrodynamic coefficients of non-spherical particles in wall-confined flows is crucial for understanding particle–fluid interactions and reliable modelling of particle motion. Under strong wall confinement, the hydrodynamic coefficients exhibit a highly nonlinear dependence on the Reynolds number, wall distance and particle orientation – posing significant modelling challenges. In this study, we propose a multi-stage physics-informed machine-learning (MSPIML) framework for modelling the drag, lift and pitching torque coefficients of a wall-bounded prolate spheroid over the explored parameter space. In the first stage, a physics-informed mixture-of-experts (PIMoE) model predicts the drag coefficient by intelligently blending empirical correlations with a data-driven statistical expert. The resulting high-fidelity drag coefficient is then injected as an auxiliary input to a second-stage model, either a deep neural network (DNN) or an additional MoE, that predicts lift and pitching torque coefficients, thereby leveraging the strong physical coupling among the three coefficients. Trained on a comprehensive dataset of 720 direct numerical simulations covering wide ranges of Reynolds number, wall distance and particle orientation, the optimal PIMoE–DNN and PIMoE–MoE configurations achieve relative errors below 2.2 % for drag, 11.4 % for lift and 7.0 % for pitching torque while maintaining excellent generalisation across the entire parameter space. Moreover, the Shapley additive explanations analysis confirms that the MSPIML framework correctly captures the physical dependencies: dominant influence of Reynolds number and strong pitching torque dependence on the drag coefficient. The MSPIML framework provides an interpretable and efficient approach to the prediction of hydrodynamic coefficients and offers substantial potential for dynamic modelling of non-spherical particles in multiphase flows.
- 4 May 2026
- Published by Cambridge University Press (CUP) in Journal of Fluid Mechanics
- Vol. 1034
Open AccessPrediction of the drag, lift and torque coefficients of non-spherical particles constrained by wall
Accurate prediction of the hydrodynamic coefficients of non-spherical particles in wall-confined flows is crucial for understanding particle–fluid interactions and reliable modelling of particle motion. Under strong wall confinement, the hydrodynamic coefficients exhibit a highly nonlinear dependence on the Reynolds number, wall distance and particle orientation – posing significant modelling challenges. In this study, we propose a multi-stage physics-informed machine-learning (MSPIML) framework for modelling the drag, lift and pitching torque coefficients of a wall-bounded prolate spheroid over the explored parameter space. In the first stage, a physics-informed mixture-of-experts (PIMoE) model predicts the drag coefficient by intelligently blending empirical correlations with a data-driven statistical expert. The resulting high-fidelity drag coefficient is then injected as an auxiliary input to a second-stage model, either a deep neural network (DNN) or an additional MoE, that predicts lift and pitching torque coefficients, thereby leveraging the strong physical coupling among the three coefficients. Trained on a comprehensive dataset of 720 direct numerical simulations covering wide ranges of Reynolds number, wall distance and particle orientation, the optimal PIMoE–DNN and PIMoE–MoE configurations achieve relative errors below 2.2 % for drag, 11.4 % for lift and 7.0 % for pitching torque while maintaining excellent generalisation across the entire parameter space. Moreover, the Shapley additive explanations analysis confirms that the MSPIML framework correctly captures the physical dependencies: dominant influence of Reynolds number and strong pitching torque dependence on the drag coefficient. The MSPIML framework provides an interpretable and efficient approach to the prediction of hydrodynamic coefficients and offers substantial potential for dynamic modelling of non-spherical particles in multiphase flows.
- 20 April 2026
- Published by Cambridge University Press (CUP) in Journal of Fluid Mechanics
- Vol. 1033
Three-stage evolution of ejecta transport in shock-induced converging gases
It is of great importance for fields such as implosion dynamics and fusion research to understand the dynamics of ejecta transport in converging gases. In this paper, the evolution of particulate flow within a cylindrically imploding system is investigated experimentally and numerically. The ejecta particles are emitted from the inner surface of a roughened Sn liner into vacuum, He and Ar gases. Dynamic images of liner implosion and ejecta transport are obtained with X-ray radiographs and multi-frame optical schlieren images. The transport of ejecta particles is simulated with a four-way coupled multiphase flow model, including modelling of gas–particle coupling and inter-particle collisions. Results reveal that the ejecta transport in shock-induced converging gases differs significantly from that in planar systems, primarily due to features such as interaction with the rebounding gas shock wave and continuous compression by the imploding liner. After being generated from the inner surface, the ejecta width undergoes an ‘expansion–compression’ variation. According to mechanisms governing ejecta–gas coupling, three distinct stages of ejecta evolution are identified: (i) post-shock transport dominated by drag and particle breakup; (ii) shock-particle interaction leading to quick reduction in particle size and rapid deceleration of the ejecta front; and (iii) dense ejecta compression governed by inter-particle collisions. Leveraging particle motion and size predictions at the ejecta front, combined with the self-similar converging shock solution, a theoretical model is established to estimate the three-stage evolution of ejecta width in a cylindrically converging system.
- 20 April 2026
- Published by Cambridge University Press (CUP) in Journal of Fluid Mechanics
- Vol. 1033
Three-stage evolution of ejecta transport in shock-induced converging gases
It is of great importance for fields such as implosion dynamics and fusion research to understand the dynamics of ejecta transport in converging gases. In this paper, the evolution of particulate flow within a cylindrically imploding system is investigated experimentally and numerically. The ejecta particles are emitted from the inner surface of a roughened Sn liner into vacuum, He and Ar gases. Dynamic images of liner implosion and ejecta transport are obtained with X-ray radiographs and multi-frame optical schlieren images. The transport of ejecta particles is simulated with a four-way coupled multiphase flow model, including modelling of gas–particle coupling and inter-particle collisions. Results reveal that the ejecta transport in shock-induced converging gases differs significantly from that in planar systems, primarily due to features such as interaction with the rebounding gas shock wave and continuous compression by the imploding liner. After being generated from the inner surface, the ejecta width undergoes an ‘expansion–compression’ variation. According to mechanisms governing ejecta–gas coupling, three distinct stages of ejecta evolution are identified: (i) post-shock transport dominated by drag and particle breakup; (ii) shock-particle interaction leading to quick reduction in particle size and rapid deceleration of the ejecta front; and (iii) dense ejecta compression governed by inter-particle collisions. Leveraging particle motion and size predictions at the ejecta front, combined with the self-similar converging shock solution, a theoretical model is established to estimate the three-stage evolution of ejecta width in a cylindrically converging system.
- 24 March 2026
- Published by Cambridge University Press (CUP) in Journal of Fluid Mechanics
- Vol. 1031
Effects of rotation on kinetic energy and enstrophy in Rayleigh–Taylor turbulence
The study of rotating Rayleigh–Taylor (RT) turbulence is of fundamental significance for geophysical processes and certain engineering applications. This work systematically investigates the effects of rotation on RT turbulence using direct numerical simulation (DNS), focusing primarily on the generation of kinetic energy and enstrophy, as well as the scale-to-scale transfer of kinetic energy. Based on the DNS results, it is demonstrated that there is a notable delay and inhibition of the mixing layer growth with enhancing rotation (quantified as a decreasing Rossby number, $Ro$ ). That is, energy conversion efficiency drops substantially, from approximately $50\,\%$ in the non-rotating case $Ro = \infty$ to only $10\,\%$ in the strong rotating case $Ro=0.1$ . This is because rotation amplifies the viscous dissipation associated with the shear stress components in the vertical direction within the mixing layer. Regarding enstrophy generation, baroclinic effects dominate during the early stage of flow evolution, while vortex stretching and tilting become the primary contributors in the later stage. Notably, the vortex stretching and tilting term is significantly suppressed by the rotation, resulting in three-dimensional RT turbulence exhibiting an enstrophy generation mechanism more akin to two-dimensional flow. Furthermore, analysis of scale-to-scale transfer of kinetic energy reveals an increased likelihood of local inverse energy transfer events under enhanced rotation. Specifically, strong rotation (e.g. $Ro=0.1$ ) results in strongly helical turbulence, which contains more high-helicity regions favourable for local inverse energy transfer. Moreover, the presence of rotation leads to more coherent and elongated flow structures and an enhanced efficiency of fluid mixing within the mixing layer.- 24 March 2026
- Published by Cambridge University Press (CUP) in Journal of Fluid Mechanics
- Vol. 1031
Effects of rotation on kinetic energy and enstrophy in Rayleigh–Taylor turbulence
The study of rotating Rayleigh–Taylor (RT) turbulence is of fundamental significance for geophysical processes and certain engineering applications. This work systematically investigates the effects of rotation on RT turbulence using direct numerical simulation (DNS), focusing primarily on the generation of kinetic energy and enstrophy, as well as the scale-to-scale transfer of kinetic energy. Based on the DNS results, it is demonstrated that there is a notable delay and inhibition of the mixing layer growth with enhancing rotation (quantified as a decreasing Rossby number, $Ro$ ). That is, energy conversion efficiency drops substantially, from approximately $50\,\%$ in the non-rotating case $Ro = \infty$ to only $10\,\%$ in the strong rotating case $Ro=0.1$ . This is because rotation amplifies the viscous dissipation associated with the shear stress components in the vertical direction within the mixing layer. Regarding enstrophy generation, baroclinic effects dominate during the early stage of flow evolution, while vortex stretching and tilting become the primary contributors in the later stage. Notably, the vortex stretching and tilting term is significantly suppressed by the rotation, resulting in three-dimensional RT turbulence exhibiting an enstrophy generation mechanism more akin to two-dimensional flow. Furthermore, analysis of scale-to-scale transfer of kinetic energy reveals an increased likelihood of local inverse energy transfer events under enhanced rotation. Specifically, strong rotation (e.g. $Ro=0.1$ ) results in strongly helical turbulence, which contains more high-helicity regions favourable for local inverse energy transfer. Moreover, the presence of rotation leads to more coherent and elongated flow structures and an enhanced efficiency of fluid mixing within the mixing layer.- 12 February 2026
- Published by Cambridge University Press (CUP) in Journal of Fluid Mechanics
- Vol. 1029
Transformations of velocity and temperature for compressible turbulent boundary layers from subsonic to hypersonic regimes
Compressible wall-bounded turbulent flows exhibit complex mean profiles because of the pronounced compressibility effects and heat transfer. We propose a hybrid transformation framework to collapse compressible mean velocity and temperature profiles onto incompressible forms through scaling each layer by its effective transformation, with the underlying mapping functions discovered via a physics-informed symbolic regression (PISR) method. The hybrid velocity transformation incorporates an intrinsic compressibility correction for the buffer layer and a PISR-derived mapping function for the logarithmic layer. For temperature, we introduce a hybrid transformation that integrates the Mach-invariant-type transformation in the viscous sublayer and a novel PISR-derived scaling in the logarithmic layer. The performance of these transformations is evaluated across compressible turbulent boundary layers with free-stream Mach numbers ranging from 0.5 to 8 and wall-to-recovery-temperature ratios ranging from 0.25 to 1. The hybrid velocity transformation outperforms Griffin–Fu–Moin transformation for the transformed mean velocity profiles, with the mean integrated percent error across the dataset decreasing from 1.67 % to 0.96 %. The hybrid temperature transformation performs better than the Mach-invariant-type and Trettel–Larsson-type transformations for mean temperature profiles. Moreover, the inverse hybrid velocity and temperature transformations can effectively predict the compressible mean velocity and temperature profiles with only wall conditions.
- 12 February 2026
- Published by Cambridge University Press (CUP) in Journal of Fluid Mechanics
- Vol. 1029
Transformations of velocity and temperature for compressible turbulent boundary layers from subsonic to hypersonic regimes
Compressible wall-bounded turbulent flows exhibit complex mean profiles because of the pronounced compressibility effects and heat transfer. We propose a hybrid transformation framework to collapse compressible mean velocity and temperature profiles onto incompressible forms through scaling each layer by its effective transformation, with the underlying mapping functions discovered via a physics-informed symbolic regression (PISR) method. The hybrid velocity transformation incorporates an intrinsic compressibility correction for the buffer layer and a PISR-derived mapping function for the logarithmic layer. For temperature, we introduce a hybrid transformation that integrates the Mach-invariant-type transformation in the viscous sublayer and a novel PISR-derived scaling in the logarithmic layer. The performance of these transformations is evaluated across compressible turbulent boundary layers with free-stream Mach numbers ranging from 0.5 to 8 and wall-to-recovery-temperature ratios ranging from 0.25 to 1. The hybrid velocity transformation outperforms Griffin–Fu–Moin transformation for the transformed mean velocity profiles, with the mean integrated percent error across the dataset decreasing from 1.67 % to 0.96 %. The hybrid temperature transformation performs better than the Mach-invariant-type and Trettel–Larsson-type transformations for mean temperature profiles. Moreover, the inverse hybrid velocity and temperature transformations can effectively predict the compressible mean velocity and temperature profiles with only wall conditions.