Secondary convection and the growth of the oceanic lithosphere

Luce Fleitout, David A. Yuen

Research output: Contribution to journalArticle

54 Scopus citations

Abstract

This paper presents a study of the evolution of the oceanic lithosphere from a thermomechanical approach. We have investigated the finite-amplitude development of secondary convection cells beneath the oceanic plates by means of the single-mode mean-field equations and the fully 2-dimensional convection equations, using finite-element techniques. Both Newtonian and non-Newtonian rheologies with highly temperature- and pressure dependences, and an activation energy of 100 kcal mol-1 have been employed. The temperature at the base of the convecting medium governs the final thickness of the lithosphere. The mean interior temperature varies only slightly during the temporal evolution. Non-Newtonian rheology has the tendency to induce oscillatory time-dependent behavior of the flow. Heat flow, topography and gravity are influenced by secondary convection in two ways. Small scale perturbations with wavelengths of around 600 km arise from the lateral thermal differences between the uprising and descending convective limbs; large-scale features are also produced as a consequence of lithospheric growth. The calculated quantities of the heat-flow topography and gravity associated with small-scale convection are typically in the range of O(HFU), O(102m), and O(10 mgal). The horizontal mean-temperature profiles from the convection model are used to calculate long wavelength geophysical observables as a function of age. Convective processes are found to reduce the rate of lithospheric thickening. Predictions from our model can fit well the observed data of heat flow, ocean floor topography and geoid offsets along fracture zones, the last data base exhibiting the most sensitivity to thermal perturbations below the lithosphere. Our calculations show that the oceanic lithosphere is able to grow continuously up to O(109 y), long past the flattening of the seafloor. We report here that the thickness of a thermally equilibrated lithosphere could reach ∼ 250 km, which lies within the appropriate range of values for the continental lithosphere, as inferred from studies in seismology, flexure observations, and secular polar motions.

Original languageEnglish (US)
Pages (from-to)181-212
Number of pages32
JournalPhysics of the Earth and Planetary Interiors
Volume36
Issue number3-4
DOIs
StatePublished - Dec 30 1984

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