1 / 15

Secondary upwelling instabilities developed in high Rayleigh number convection

Secondary upwelling instabilities developed in high Rayleigh number convection. Fabien Dubuffet 1 , M.S. Murphy 2 , Ludek Vecsey 3 , Erik O. Sevre 1 and David A. Yuen 1.

zarita
Télécharger la présentation

Secondary upwelling instabilities developed in high Rayleigh number convection

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Secondary upwelling instabilities developed in high Rayleigh number convection Fabien Dubuffet1, M.S. Murphy2, Ludek Vecsey3, Erik O. Sevre1 and David A. Yuen1 1 Department of Geology and Geophysics and Minnesota Supercomputing Institute, University of Minnesota, Minneapolis, MN 55415-0227, USA. 2 Department of Geology, Colby College, Waterville, ME 04901, USA. 3 Department of Geophysics, Charles University, 1800 Prague 8, Czech Republic.

  2. Whitehead's Laboratory Experiments The behavior observed by Skillbeck and Whitehead (1978) when a fluid of lower density and lower viscosity was injected into a fluid of higher density and higher viscosity at an angle of 25 degrees and allowed to propogate for two minutes.Figure courtesy of Jack Whitehead

  3. Apparatus constructed by Whitehead in 1982 to conduct his second series of experiments with tilted conduits. The rotating apparatus in the upper portion of the tank creates a zone of shear that bends the conduit as it flows upward. Resulting shadowgraph of instabilities forming from a conduit

  4. The numerical models • Boussinesq approximation. • Infinite Prandtl Number • 2-D model: • - two-dimensional axisymmetric model in a spherical shell (core radius 0.55). • fourth-order finite-difference method to solve for the vorticity, stream function, and the temperature field. • up to 3400 x 500 grid points. • 3-D model: • Cartesian geometry ( aspect ratio 3). • Stokes equation : Fast Fourier transform along the horizontal axis and finite differences. • Temperature equation : A.D.I. • up to 385 x 385 x 385 grid points.

  5. Ra = 3x106 Ra = 3x107

  6. Ra = 3x108 Ra = 109

  7. Ra = 3x109 time

  8. Ra = 5x109 Ra = 1010

  9. Ra = 3x108

  10. Zoom in

  11. Ra = 5x108

  12. Variable thermal conductivity (a = 0.9) Ra = 106

  13. Wavelength Argument - There is no unique wavelength but a broadband spectrum of possible folding wavelengths. - The variations of the bandwidth will be used to constrain the possible range of secondary folding instabilities

  14. Major islands of the state of Hawaii Figure modified from Cox (1999)

More Related