Characterization of mantle convection experiments using two-point correlation functions

Snapshots of the temperature T(r,ϕ,t), horizontal flow velocity u(r,ϕ,t), and radial flow velocity w(r, ϕ, t) obtained from numerical convection experiments of time-dependent flows in annular cylindrical geometry are taken to be samples of stationary, rotationally invariant random fields. For such a field ƒ(r,r2 ϕ, t), the spatio-temporal two-point correlation function, Cƒƒ (r, r1, Δ, t*), is constructed by averaging over rotational transformations of this ensemble. To assess the structural differences among mantle convection experiments we construct three spatial subfunctions of Cƒƒ (r, r1, Δ, t*) : the rms variation, σƒ (r), the radial correlation function, Rƒ (r,r1), and the angular correlation function, Aƒ(r, Δ). Rƒ (r,r1) and Aƒ(r,Δ) are symmetric about the loci r = r1 and Δ=0, respectively, where they achieve their maximum value of unity. The falloff of Rƒ and Aƒ away from their symmetry axes can be quantified by a correlation length ρƒ(r) and a correlation angle αƒ(r), which we define to be the half widths of the central peaks at the correlation level 0.75. The behavior of ρƒ is a diagnostic of radial structure, while αƒ measures average plume width. We have used two-point correlation functions of the temperature field (T-diagnostics) and flow velocity fields (V-diagnostics) to quantify some important aspects of mantle convection experiments. We explore the dependence of different correlation diagnostics on Rayleigh number, internal heating rate, and depth- and temperature-dependent viscosity. For isoviscous flows in an annulus, we show how radial averages of σT, ρT, and αT scale with Rayleigh number for various internal heating rates. A break in the power-law relationship at the transition from steady to time-dependent regimes is evident for ρT and αT but not for σT or the Nusselt number. A rapid tenfold to thirtyfold viscosity increase with depth yields weakly stratified flows, quantified by aw, which is a measure of radial flux. The horizontal flux diagnostic, σu, reveals that the flow organization is sensitive to the depth of the viscosity increase. A jump at middepth induces a significant horizontal return flow at the base of the upper layer, absent in models with a jump at quarter-depth. We illustrate that T-diagnostics, which are more easily relatable to geophysical observables, can serve as proxies for the V-diagnostics. A viscosity increase with depth is evident as an increase in the T-diagnostics in the high-viscosity region. For numerical experiments with a temperature-dependent rheology we employ a mobilization scheme for the upper boundary layer. Temperature dependence does not appreciably perturb the σ-diagnostics or αT in the convecting interior. Changes in the radial correlation length are twofold. First, the greater viscosity of cold downwellings leads to an increase in height and width of the radial correlation maximum near the top. Second, the increase in ρT associated with a viscosity jump is markedly reduced. The latter effect can be explained by weaker, less stationary hot upwellings, mobilized by the temperature-dependent rheology and disrupted by the cold, high-viscosity downwellings.

[1]  T. Jordan Structural geology of the Earth's interior. , 1979, Proceedings of the National Academy of Sciences of the United States of America.

[2]  L. Howard Convection at high Rayleigh number , 1966 .

[3]  M. Ashby,et al.  Micromechanisms of flow and fracture, and their relevance to the rheology of the upper mantle , 1978, Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences.

[4]  Robert W. Clayton,et al.  Lower mantle heterogeneity, dynamic topography and the geoid , 1985, Nature.

[5]  Guy Masters,et al.  An inversion for radial viscosity structure using seismic tomography , 1992 .

[6]  Wei-jia Su,et al.  Degree 12 model of shear velocity heterogeneity in the mantle , 1994 .

[7]  Ulrich R. Christensen,et al.  Convection with pressure- and temperature-dependent non-Newtonian rheology , 1984 .

[8]  L. Sirovich,et al.  Probability distribution functions in turbulent convection , 1991 .

[9]  Patrice Weber,et al.  Intermittent layered convection in a model mantle with an endothermic phase change at 670 km , 1991, Nature.

[10]  Mark J. Beran,et al.  Statistical Continuum Theories , 1968 .

[11]  David J. Stevenson,et al.  Effects of an endothermic phase transition at 670 km depth in a spherical model of convection in the Earth's mantle , 1993, Nature.

[12]  M. Gurnis,et al.  Numerical study of high Rayleigh number convection in a medium with depth-dependent viscosity , 1986 .

[13]  S. Honda The RMS residual temperature in the convecting mantle and seismic heterogeneities. , 1987 .

[14]  S. Zhong,et al.  Generation of Long Wavelength Heterogeneity in the Mantle by the Dynamic Interaction Between Plates and Convection (Paper 91GL00823) 581 , 1991 .

[15]  D. Yuen,et al.  Dynamical consequences of depth-dependent thermal expansivity and viscosity on mantle circulations and thermal structure , 1993 .

[16]  M. Gurnis,et al.  Viscous flow model of a subduction zone with a faulted lithosphere: Long and short wavelength topography, gravity and geoid , 1992 .

[17]  Frank M. Richter,et al.  Convection experiments in fluids with highly temperature-dependent viscosity and the thermal evolution of the planets , 1982 .

[18]  P. Richards,et al.  Borovoye Geophysical Observatory, Kazakhstan , 1992 .

[19]  Yuen,et al.  Comparison of steady-state and strongly chaotic thermal convection at high Rayleigh number. , 1992, Physical review. A, Atomic, molecular, and optical physics.

[20]  G. Jarvis The Unifying Role of Aspect Ratio In Cylindrical Models of Mantle Convection With Varying Degrees of Curvature , 1994 .

[21]  David A. Yuen,et al.  Transition to hard turbulence in thermal convection at infinite Prandtl number , 1990 .

[22]  Solomon,et al.  Thermal boundary layers and heat flux in turbulent convection: The role of recirculating flows. , 1991, Physical review. A, Atomic, molecular, and optical physics.

[23]  Bradford H. Hager,et al.  Conman: vectorizing a finite element code for incompressible two-dimensional convection in the Earth's mantle , 1990 .

[24]  T. Jordan,et al.  Comparisons Between Seismic Earth Structures and Mantle Flow Models Based on Radial Correlation Functions , 1993, Science.

[25]  G. Schubert,et al.  Three‐dimensional spherical models of layered and whole mantle convection , 1993 .

[26]  T. Jordan,et al.  Stochastic analysis of mantle convection experiments using two‐point correlation functions , 1994 .

[27]  T. Jordan,et al.  Continents as a chemical boundary layer , 1981, Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences.

[28]  Adolf Ebel,et al.  Time-dependent thermal convection - a possible explanation for a multiscale flow in the Earth's mantle , 1988 .

[29]  Libchaber,et al.  Transitions to turbulence in helium gas. , 1987, Physical review. A, General physics.

[30]  S. Zaleski,et al.  Scaling of hard thermal turbulence in Rayleigh-Bénard convection , 1989, Journal of Fluid Mechanics.

[31]  G. Jarvis Effects of curvature on two‐dimensional models of mantle convection: Cylindrical polar coordinates , 1993 .

[32]  Rosner,et al.  Numerical simulations of soft and hard turbulence: Preliminary results for two-dimensional convection. , 1990, Physical review letters.

[33]  W. Peltier,et al.  Lateral heterogeneity in the convecting mantle , 1986 .

[34]  Shijie Zhong,et al.  Dynamic feedback between a continentlike raft and thermal convection , 1993 .

[35]  A. Vincent,et al.  The spatial structure and statistical properties of homogeneous turbulence , 1991, Journal of Fluid Mechanics.

[36]  W. Peltier,et al.  Mantle phase transitions and layered chaotic convection , 1992 .

[37]  David J. Stevenson,et al.  Effects of multiple phase transitions in a three-dimensional spherical model of convection in Earth's mantle , 1994 .

[38]  T. Tanimoto Long-wavelength S-wave velocity structure throughout the mantle , 1990 .

[39]  D. Yuen,et al.  Convective mixing and the fine structure of mantle heterogeneity , 1984 .

[40]  G. Jarvis,et al.  Geometrical effects of curvature in axisymmetric spherical models of mantle convection , 1994 .

[41]  D. Thomson,et al.  Some comments on magnetotelluric response function estimation , 1989 .

[42]  T. Lay Structure of the core‐mantle transition zone , 1989 .

[43]  G. M. Corcos,et al.  A boundary layer model for mantle convection with surface plates , 1980 .