Export citation

Export citation

Choose format for download:

Download Citation
  • Access by Xinjiang University

Small scale quasigeostrophic convective turbulence at large Rayleigh number

Tobias G. Oliver1, Adrienne S. Jacobi1, Keith Julien2, and Michael A. Calkins1

  • 1Department of Physics, University of Colorado, Boulder, Colorado 80309, USA
  • 2Department of Applied Mathematics, University of Colorado, Boulder, Colorado 80309, USA

Phys. Rev. Fluids 8, 093502 – Published 12 September, 2023

DOI: https://doi.org/10.1103/PhysRevFluids.8.093502

Abstract

A numerical investigation of an asymptotically reduced model for quasigeostrophic Rayleigh-Bénard convection is conducted in which the depth-averaged flows are numerically suppressed by modifying the governing equations. At the largest accessible values of the Rayleigh number Ra, the Reynolds number and Nusselt number show evidence of approaching the diffusion-free scalings of ReRaE/Pr and NuPr1/2Ra3/2E2, respectively, where E is the Ekman number and Pr is the Prandtl number. For large Ra, the presence of depth-invariant flows, such as large-scale vortices, yield heat and momentum transport scalings that exceed those of the diffusion-free scaling laws. The Taylor microscale does not vary significantly with increasing Ra, whereas the integral length scale grows weakly. The computed length scales remain O(1) with respect to the linearly unstable critical wave number; we therefore conclude that these scales remain viscously controlled. We do not find a point-wise Coriolis-inertia-Archimedean (CIA) force balance in the turbulent regime; interior dynamics are instead dominated by horizontal advection (inertia), vortex stretching (Coriolis) and the vertical pressure gradient. A secondary, subdominant balance between the Archimedean buoyancy force and the viscous force occurs in the interior and the ratio of the root mean square (rms) of these two forces is found to approach unity with increasing Ra. This secondary balance is attributed to the turbulent fluid interior acting as the dominant control on the heat transport. These findings indicate that a pointwise CIA balance does not occur in the high Rayleigh number regime of quasigeostrophic convection in the plane layer geometry. Instead, simulations are characterized by what may be termed a nonlocal CIA balance in which the buoyancy force is dominant within the thermal boundary layers and is spatially separated from the interior Coriolis and inertial forces.

Physics Subject Headings (PhySH)

Article Text

References (37)

  1. S. Stanley and G. A. Glatzmaier, Dynamo models for planets other than earth, Space Sci. Rev. 152, 617 (2010).
  2. C. A. Jones, Planetary magnetic fields and fluid dynamos, Annu. Rev. Fluid Mech. 43, 583 (2011).
  3. P. H. Roberts and E. M. King, On the genesis of the Earth's magnetism, Rep. Prog. Phys. 76, 096801 (2013).
  4. J. M. Aurnou, M. A. Calkins, J. S. Cheng, K. Julien, E. M. King, D. Nieves, K. M. Soderlund, and S. Stellmach, Rotating convective turbulence in Earth and planetary cores, Phys. Earth Planet. Inter. 246, 52 (2015).
  5. P. Charbonneau, Solar dynamo theory, Annu. Rev. Astron. Astrophys. 52, 251 (2014).
  6. M. Heimpel, T. Gastine, and J. Wicht, Simulation of deep-seated zonal jets and shallow vortices in gas giant atmospheres, Nat. Geosci. 9, 19 (2016).
  7. L. Siegelman, P. Klein, A. P. Ingersoll, S. P. Ewald, W. R. Young, A. Bracco, A. Mura, A. Adriani, D. Grassi, C. Plainaki et al., Moist convection drives an upscale energy transfer at Jovian high latitudes, Nat. Phys. 18, 357 (2022).
  8. R. E. Ecke and J. J. Niemela, Heat Transport in the Geostrophic Regime of Rotating Rayleigh-Bénard Convection, Phys. Rev. Lett. 113, 114301 (2014).
  9. J. S. Cheng, S. Stellmach, A. Ribeiro, A. Grannan, E. M. King, and J. M. Aurnou, Laboratory-numerical models of rapidly rotating convection in planetary cores, Geophys. J. Int. 201, 1 (2015).
  10. M. Madonia, A. J. A. Guzmán, H. J. H. Clercx, and R. P. J. Kunnen, Velocimetry in rapidly rotating convection: Spatial correlations, flow structures and length scales (a), Europhys. Lett. 135, 54002 (2021).
  11. T. Vogt, S. Horn, and J. M. Aurnou, Oscillatory thermal–inertial flows in liquid metal rotating convection, J. Fluid Mech. 911, A5 (2021).
  12. T. Gastine, J. Wicht, and J. Aubert, Scaling regimes in spherical shell rotating convection, J. Fluid Mech. 808, 690 (2016).
  13. A. J. Aguirre Guzmán, M. Madonia, J. S. Cheng, O. Ostilla-Mónico, H. J. H. Clercx, and R. P. J. Kunnen, Force balance in rapidly rotating Rayleigh-Bènard convection, J. Fluid Mech. 928, A16 (2021).
  14. M. Yan and M. A. Calkins, Asymptotic behaviour of rotating convection-driven dynamos in the plane layer geometry, J. Fluid Mech. 951, A24 (2022).
  15. K. Julien, E. Knobloch, and J. Werne, A new class of equations for rotationally constrained flows, Theor. Comput. Fluid Dyn. 11, 251 (1998).
  16. S. Stellmach, M. Lischper, K. Julien, G. Vasil, J. S. Cheng, A. Ribeiro, E. M. King, and J. M. Aurnou, Approaching the Asymptotic Regime of Rapidly Rotating Convection: Boundary Layers versus Interior Dynamics, Phys. Rev. Lett. 113, 254501 (2014).
  17. M. Plumley, K. Julien, P. Marti, and S. Stellmach, The effects of Ekman pumping on quasi-geostrophic Rayleigh-Bénard convection, J. Fluid Mech. 803, 51 (2016).
  18. S. Maffei, M. J. Krouss, K. Julien, and M. A. Calkins, On the inverse cascade and flow speed scaling behaviour in rapidly rotating Rayleigh–Bénard convection, J. Fluid Mech. 913, A18 (2021).
  19. K. Julien, A. M. Rubio, I. Grooms, and E. Knobloch, Statistical and physical balances in low Rossby number Rayleigh-Bénard convection, Geophys. Astrophys. Fluid Dyn. 106, 392 (2012).
  20. A. M. Rubio, K. Julien, E. Knobloch, and J. B. Weiss, Upscale Energy Transfer in Three-Dimensional Rapidly Rotating Turbulent Convection, Phys. Rev. Lett. 112, 144501 (2014).
  21. B. Favier, L. J. Silvers, and M. R. E. Proctor, Inverse cascade and symmetry breaking in rapidly rotating Boussinesq convection, Phys. Fluids 26, 096605 (2014).
  22. C. Guervilly, D. W. Hughes, and C. A. Jones, Large-scale vortices in rapidly rotating Rayleigh-Bénard convection, J. Fluid Mech. 758, 407 (2014).
  23. J. A. Nicoski, M. Yan, and M. A. Calkins, Quasistatic magnetoconvection with a tilted magnetic field, Phys. Rev. Fluids 7, 043504 (2022).
  24. K. Julien, E. Knobloch, A. M. Rubio, and G. M. Vasil, Heat Transport in Low-Rossby-Number Rayleigh-Bénard Convection, Phys. Rev. Lett. 109, 254503 (2012).
  25. C. Guervilly, P. Cardin, and N. Schaeffer, Turbulent convective length scale in planetary cores, Nature (London) 570, 368 (2019).
  26. S. B. Pope, Turbulent Flows (Cambridge University Press, Cambridge, 2000).
  27. C. A. Jones, Thermal and compositional convection in the outer core, in Treatise on Geophysics, edited by G. Schubert (Elsevier, 2015), Vol. 8, pp. 115–159.
  28. J. M. Aurnou, S. Horn, and K. Julien, Connections between nonrotating, slowly rotating, and rapidly rotating turbulent convection transport scalings, Phys. Rev. Res. 2, 043115 (2020).
  29. M. Sprague, K. Julien, E. Knobloch, and J. Werne, Numerical simulation of an asymptotically reduced system for rotationally constrained convection, J. Fluid Mech. 551, 141 (2006).
  30. P. Marti, M. A. Calkins, and K. Julien, A computationally efficient spectral method for modeling core dynamics, Geochem., Geophys., Geosyst. 17, 3031 (2016).
  31. G. K. Vallis, Atmospheric and Oceanic Fluid Dynamics (Cambridge University Press, Cambridge, 2006).
  32. S. Chandrasekhar, Hydrodynamic and Hydromagnetic Stability (Oxford University Press, UK, 1961).
  33. M. Yan and M. A. Calkins, Strong large scale magnetic fields in rotating convection-driven dynamos: The important role of magnetic diffusion, Phys. Rev. Res. 4, L012026 (2022).
  34. N. Schaeffer, D. Jault, H.-C. Nataf, and A. Fournier, Turbulent geodynamo simulations: a leap towards Earth's core, Geophys. J. Int. 211, 1 (2017).
  35. R. J. A. M. Stevens, A. Blass, X. Zhu, R. Verzicco, and D. Lohse, Turbulent thermal superstructures in Rayleigh-Bénard convection, Phys. Rev. Fluids 3, 041501(R) (2018).
  36. M. Yan, S. M. Tobias, and M. A. Calkins, Scaling behaviour of small-scale dynamos driven by Rayleigh–Bénard convection, J. Fluid Mech. 915, A15 (2021).
  37. T. Gastine and J. M. Aurnou, Latitudinal regionalization of rotating spherical shell convection, J. Fluid Mech. 954, R1 (2023).

Outline

Information

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation