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Baroclinic eddies

Dr Shanshan Ding

Visitor

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Geophysical and Astrophysical Fluid Dynamics
shanshan.ding@physics.ox.ac.uk
Atmospheric Physics Clarendon Laboratory, room 209E
  • About
  • Publications

Vortex patterns in rapidly rotating Rayleigh–Bénard convection under spatial periodic forcing

Journal of Fluid Mechanics Cambridge University Press (CUP) 950 (2022) R1

Authors:

Shan-Shan Ding, Hong-Lin Zhang, Dong-Tian Chen, Jin-Qiang Zhong

Abstract:

Pattern-forming with externally imposed symmetry is ubiquitous in nature but little studied. We present experimental studies of pattern formation and selection by spatial periodic forcing in rapidly rotating convection. When periodic topographic structures are constructed on the heated boundary, they modulate the local temperature and velocity fields. Symmetric convection patterns in the form of regular vortex lattices are observed near the onset of convection, when the periodicity of the external forcing is set close to the intrinsic vortex spacing. We show that the new patterns arise as a dynamical process of imperfect bifurcation which is well described by a Ginzburg–Landau-like model. We explore the phase diagram of buoyancy strength and periodicity of external forcing to find the optimal experimental settings for which the vortex patterns best match that of the external forcing.

Neutrally- and Stably-Stratified Boundary Layers Adjustments to a Step Change in Surface Roughness

(2022)

Authors:

Shan-Shan Ding, Marco Placidi, Matteo Carpentieri, Alan Robins

Inverse centrifugal effect induced by collective motion of vortices in rotating thermal convection

Nature Communications Nature Research 12:1 (2021) 5585

Authors:

Shan-Shan Ding, Kai Leong Chong, Jun-Qiang Shi, Guang-Yu Ding, Hao-Yuan Lu, Ke-Qing Xia, Jin-Qiang Zhong

Abstract:

AbstractWhen a fluid system is subject to strong rotation, centrifugal fluid motion is expected, i.e., denser (lighter) fluid moves outward (inward) from (toward) the axis of rotation. Here we demonstrate, both experimentally and numerically, the existence of an unexpected outward motion of warm and lighter vortices in rotating thermal convection. This anomalous vortex motion occurs under rapid rotations when the centrifugal buoyancy is sufficiently strong to induce a symmetry-breaking in the vorticity field, i.e., the vorticity of the cold anticyclones overrides that of the warm cyclones. We show that through hydrodynamic interactions the densely distributed vortices can self-aggregate into coherent clusters and exhibit collective motion in this flow regime. Interestingly, the correlation of the vortex velocity fluctuations within a cluster is scale-free, with the correlation length being proportional ( ≈ 30%) to the cluster length. Such long-range correlation leads to the counterintuitive collective outward motion of warm vortices. Our study brings insights into the vortex dynamics that are widely present in nature.

Vortices as Brownian particles in turbulent flows.

Science advances 6:34 (2020) eaaz1110

Authors:

Kai Leong Chong, Jun-Qiang Shi, Guang-Yu Ding, Shan-Shan Ding, Hao-Yuan Lu, Jin-Qiang Zhong, Ke-Qing Xia

Abstract:

Brownian motion of particles in fluid is the most common form of collective behavior in physical and biological systems. Here, we demonstrate through both experiment and numerical simulation that the movement of vortices in a rotating turbulent convective flow resembles that of inertial Brownian particles, i.e., they initially move ballistically and then diffusively after certain critical time. Moreover, the transition from ballistic to diffusive behaviors is direct, as predicted by Langevin, without first going through the hydrodynamic memory regime. The transitional timescale and the diffusivity of the vortices can be collapsed excellently onto a master curve for all explored parameters. In the spatial domain, however, the vortices exhibit organized structures, as if they are performing tethered random motion. Our results imply that the convective vortices have inertia-induced memory such that their short-term movement can be predicted and their motion can be well described in the framework of Brownian motions.

Fine vortex structure and flow transition to the geostrophic regime in rotating Rayleigh-Bénard convection

Physical Review Fluids American Physical Society (APS) 5:1 (2020) 011501

Authors:

Jun-Qiang Shi, Hao-Yuan Lu, Shan-Shan Ding, Jin-Qiang Zhong

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