arXiv subjects

Shijun Chu

Publications and source records attributed to Shijun Chu.

5 recordsLinked to original sources

arXiv2026

Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations

We study tidal flows in the convective envelopes of rotating, magnetised fluid bodies, such as low-mass stars and giant planets. In well-mixed convective regions, (magneto-)inertial waves are linearly excited by tidal forcing, and their dissipation can dominantly drive spin and orbital evolution in many close star-planet and binary star systems. We perform linear magnetohydrodynamic calculations of wavelike tides in spherical-shell geometry of a tidally-forced, rotating, incompressible, viscous and non-ideal magnetised fluid. Our calculations consider the widest range of magnetic field configurations to date (including both aligned and misaligned dipole fields, free-decay dipole and quadrupole fields, azimuthal "Malkus fields" and mixed poloidal-toroidal "Prendergast fields") to analyse the effects of magnetic fields on the wavelike response and dissipation. We find that the tidal response at a given frequency depends strongly on both magnetic field strength and geometry. Magnetic fields with strong poloidal components modify the flow more efficiently and introduce high-frequency Alfv\'enic resonances associated with weakly damped eigenmodes. When an enhanced (turbulent) viscosity is adopted, we find that viscous dissipation remains comparable to Ohmic dissipation for strong fields, in contrast to previous studies in which Ohmic dissipation was argued to dominate. We also explore the variation in magnetic effects as the shell thickness, magnetic Prandtl and Ekman numbers are varied. Finally, the frequency-averaged tidal power is found to be largely insensitive to the magnetic field in most cases, though significant deviations are found for free-decay fields. Our results have important implications for the tidal evolution of magnetised, rotating stars and planets.

astro-ph.EP↗

arXiv2025

Optimal body force for heat transfer in turbulent vertical heated pipe flow

The vertical heated-pipe is widely used in thermal engineering applications, as buoyancy can help drive a flow, but several flow regimes are possible: shear-driven turbulence, laminarised flow, and convective turbulence. Steady velocity fields that maximise heat transfer have previously been calculated for heated pipe flow, but were calculated independently of buoyancy forces, and hence independently of the flow regime and time-dependent dynamics of the flow. In this work, a variational method is applied to find an optimal body force of limited magnitude that maximises heat transfer for the vertical arrangement, with the velocity field constrained by the full governing equations. In our calculations, mostly at Re=3000, it is found that streamwise-independent rolls remain optimal, as in previous steady optimisations, but that the optimal number of rolls and their radial position are dependent on the flow regime. Surprisingly, while it is generally assumed that turbulence enhances heat transfer, for the strongly forced case, time-dependence typically leads to a reduction. Beyond offering potential improvement through the targeting of the roll configuration for this application, wider implications are that optimisations under the steady flow assumption may overestimate improvements in heat transfer, and that strategies that simply aim to induce turbulence may not necessarily be efficient in enhancing heat transfer either. Including time-dependence and the full governing equations in the optimisation is challenging but offers further enhancement and improved reliability in prediction.

physics.flu-dyn↗

arXiv2025

Modelling the transition from shear-driven turbulence to convective turbulence in a vertical heated pipe

Heated pipe flow is widely used in thermal engineering applications, but the presence of buoyancy force can cause intermittency, or multiple flow states at the same parameter values. Such changes in the flow lead to substantial changes in its heat transfer properties and thereby significant changes in the axial temperature gradient. We therefore introduce a model that features a time-dependent background axial temperature gradient, and consider two temperature boundary conditions -- fixed temperature difference and fixed boundary heat flux. Direct numerical simulations (DNS) are based on the pseudo-spectral framework, and good agreement is achieved between present numerical results and experimental results. The code extends openpipeflow.org and is available at the website. The effect of the axially periodic domain on flow dynamics and heat transfer is examined, using pipes of length L=5D and L=25D. Provided that the flow is fully turbulent, results show close agreement for the mean flow and temperature profiles, and only slight differences in root-mean-square fluctuations. When the flow shows spatial intermittency, heat transfer tends to be overestimated using a short pipe, as shear turbulence fills the domain. This is particularly important when shear turbulence starts to be suppressed at intermediate buoyancy numbers. Finally, at such intermediate buoyancy numbers, we confirm that the decay of localised shear turbulence in the heated pipe flow follows a memoryless process, similar to that in isothermal flow. While isothermal flow then laminarises, convective turbulence in the heated flow can intermittently trigger bursts of shear-like turbulence.

physics.flu-dyn↗

arXiv2024

Laminarising turbulent pipe flow by linear and nonlinear optimisation

It has been observed that flattening the mean velocity profile of pipe flow by body force can laminarise turbulence, a promising means to reduce frictional drag substantially. To explore whether there is a more efficient body force to eliminate turbulence, we consider time-independent active body forces with varying spatial dependencies. Results confirm that when using an active force, a flattened forced laminar profile is needed to eliminate turbulence, and that a purely streamwise body force is best for laminarisation. While these results required an expensive nonlinear optimisation, it was also observed that the optimal forced profile exhibits reduced linear transient growth (TG). To determine whether the reduction of linear TG alone is a sufficient target for the laminarisation of turbulence, a linear Lagrange Multiplier technique is used to minimise TG of perturbations to the forced laminar profile. The optimal velocity profiles reveal that TG for each azimuthal wavenumber strongly depends on the radial velocity gradient at some specific radial interval. The optimal velocity profile obtained by minimising TG of perturbations of azimuthal wavenumber m = 1 is shown to be able to eliminate turbulence at Re = 2400, but a more effective reduction of TG, including perturbations of higher m, is needed for laminarisation at higher Reynolds number Re = 3000. The streaks formed with the flattened forced laminar profile reveal the mechanism of laminarisation: it is found that the lift-up mechanism in the more flattened forced laminar profile creates a lower streak (i.e. closer to the wall) that is more stable, so that turbulence is harder to maintain through streak instability. Further numerical experiments by disturbing a periodic orbit validated that the breakdown of turbulence self-sustaining mechanisms is mainly caused by suppression of the formation of streaks.

physics.flu-dyn↗

arXiv2024

The minimal seed for transition to convective turbulence in heated pipe flow

It is well known that buoyancy suppresses, and can even laminarise turbulence in upward heated pipe flow. Heat transfer seriously deteriorates in this case. Through a new DNS model, we confirm that the deteriorated heat transfer within convective turbulence is related to a lack of near-wall rolls, which leads to a weak mixing between the flow near the wall and centre of pipe. Having surveyed the fundamental properties of the system, we perform a nonlinear nonmodal stability analysis. it is found that, the minimal seed becomes thinner and closer to the wall, with increase of buoyancy number C. Most importantly, we show that the critical initial energy required to trigger shear-driven turbulence keeps increasing, implying that attempts to artificially trigger it may not be an efficient means to improve heat transfer at larger C. The new minimal seed, found at C=6, is localised in streamwise direction and is active in the centre of pipe. To find this branch of optimal, we took advantage of a window of linear stability. While the nonlinear optimal causes transition to convective turbulence directly at this and larger C, transition via the linear instability passes via a travelling wave or periodic orbit solutions. Detailed analysis of the periodic solution reveals three stages: growth of the unstable eigenfunction, the formation of streaks, and the decay of streaks due to suppression of the instability. Flow visualization at C up to 10 also show similar features, suggesting that convective turbulence is sustained by these three typical processes.

physics.flu-dyn↗