4.8 Article

Model of Convective Taylor Columns in Rotating Rayleigh-Benard Convection

Journal

PHYSICAL REVIEW LETTERS
Volume 104, Issue 22, Pages -

Publisher

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.104.224501

Keywords

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Funding

  1. NSF FRG [DMS-0855010, DMS-0854841]
  2. Division Of Mathematical Sciences
  3. Direct For Mathematical & Physical Scien [0854841, 0855010] Funding Source: National Science Foundation

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Observations, and laboratory and numerical studies, of fluid flows with strong rotation and thermal forcing often show long-lived convective Taylor columns (CTCs) which carry a large portion of the vertical heat and mass fluxes. However, owing to experimental and numerical challenges, these structures remain poorly understood. Here we present a nonlinear, analytical multiscale model of CTCs in the context of rotating Rayleigh-Benard convection that successfully matches numerical simulations and provides a new multiscale interpretation of the Taylor-Proudman constraint.

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