Abstract

Measurements of the velocity field associated with plumes rising through a viscous fluid are performed using stereoscopic Particle-Image Velocimetry in the Rayleigh number range 4.4 × 105 − 6.4 × 105. The experimental model is analogous to a mantle plume rising from the core-mantle boundary to the base of the lithosphere. The behaviour of the plume is studied throughout its life cycle, which is broken up into four stages; the Formation Stage, when the plume forms; the Rising Stage, when the plume rises through the fluid; the Spreading Stage, when the plume reaches the surface and spreads; and finally the Declining Stage, when the heat source has been removed and the plume weakens. The latter three stages are examined in terms of the Finite-Time Lyapunov Exponent fields and the advection of passive tracers throughout the flow. The temperature at the heater and near the fluid surface are measured using thermocouples to infer how the presence of a mantle plume would produce excess temperature near the lithosphere throughout the various stages of its life cycle. In all experiments a time lag is observed between the removal of the heat source and the decline in the excess temperature near the surface, which is proportional to the rise time. A simple analytical model is presented, which suggests that under mantle conditions (i.e. negligible thermal diffusion), the relationship between the time lag and the rise time is robust and independent of the Rayleigh number; however, the constant of proportionality is closer to unity in the absence of diffusion. Once the heat source is removed, the excess temperature near the surface declines exponentially at a rate that is inversely proportional to the rise time. The implications of this result are discussed in terms of the decline in volcanism in the Louisville hotspot chain over the past 20 Ma. The rise velocity of material in the plume is examined; the rise velocity is found to vary significantly with the plume height in a manner that is inconsistent with many of the common semi-analytical models of thermal plumes in the literature. It is also argued that this height-dependency will cause estimates of the rise velocity based on the decay series of Uranium isotopes to significantly underestimate the true value.

Highlights

  • Mantle plumes are columns of hot material that rise from a thermal boundary in the mantle and are thought to be a cause of intraplate volcanism (Morgan 1971; Richards et al 1989)

  • The geochemical signature of Ocean Island Basalts (OIBs), which are generally attributed to the presence of a mantle plume, is distinct from that of Mid-Ocean Ridge Basalts (MORBs) which are derived from the depleted upper mantle (Hofmann 1997; Hart et al 1992)

  • In order to fully understand the origin of the geochemical signature of OIBs and to use this data to gain insight into the chemical composition of the mantle, it is first necessary to understand the behaviour of a thermal plume as it passes through a fluid and reaches the surface

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Summary

Introduction

Mantle plumes are columns of hot material that rise from a thermal boundary in the mantle and are thought to be a cause of intraplate volcanism (Morgan 1971; Richards et al 1989). The behaviour of plumes is important in terms of understanding the heat flow within the Earth’s interior (Lay et al 2008) and can provide insight into the mixing history and chemical composition of the mantle (Kellogg 1992). In order to fully understand the origin of the geochemical signature of OIBs and to use this data to gain insight into the chemical composition of the mantle, it is first necessary to understand the behaviour of a thermal plume as it passes through a fluid and reaches the surface. The behaviour of a thermal plume and the nature of heat flow in the mantle are controlled by the Rayleigh number, Ra = ρα T g D3 (1). The Rayleigh number in the mantle is thought to be of the order of ∼107,

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