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Evolution of Staircase Structures in Diffusive Convection
Published on: September 5, 2018
Evolving mantle convection from bottom up to top down
Ross N Mitchell1, Michael Brown2, Thomas M Gernon3
1State Key Laboratory of Lithospheric Evolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, China.
This study explores how heat moves through Earth's mantle by looking at whether convection is driven from the bottom up, the top down, or a balance of both. The research finds that convection is not always force balanced and can be influenced by thermal conditions at the core-mantle and lithosphere-asthenosphere boundaries. Bottom-up convection is linked to plume ascent, while top-down convection is tied to subduction. The study suggests that convection can be symmetric when these forces are balanced but does not confirm whether one mode dominates. The authors propose that the dominant mode of convection may change over time depending on boundary conditions.
Area of Science:
- Geodynamics within Earth sciences
- Plate tectonics and mantle processes
- Convection modeling in planetary geology
Background:
The Earth's mantle is a dynamic layer where heat transfer occurs through convection. While convection is generally mass balanced, the balance of buoyancy forces is not necessarily fixed. Prior research has shown that convection can be driven by either positive or negative buoyancy forces, depending on the thermal conditions at the top and bottom boundaries of the mantle. The core-mantle boundary and the lithosphere-asthenosphere boundary are key regions influencing these forces. Bottom-up convection is associated with plume ascent, while top-down convection is linked to subduction processes. However, it remains unclear whether mantle convection is symmetric, dominantly top-down, dominantly bottom-up, or time-dependent. This uncertainty has motivated further investigation into the mechanisms and balance of mantle convection.
Purpose Of The Study:
This study aims to clarify the nature of mantle convection by examining whether it is symmetric, dominantly top-down, dominantly bottom-up, or time-dependent. The specific problem addressed is the lack of consensus on the dominant mode of convection in Earth's mantle. The motivation stems from the need to better understand the forces driving mantle dynamics and their implications for surface processes like plate tectonics. The study seeks to determine whether convection is driven primarily by plume ascent, subduction, or a balance of both. By analyzing the balance of buoyancy forces, the research aims to shed light on the mechanisms governing mantle convection and how they evolve over time.
Main Methods:
The study employs a theoretical framework to analyze the balance of buoyancy forces in mantle convection. It considers the thermal conditions at the core-mantle boundary and the lithosphere-asthenosphere boundary as key factors influencing convection. The approach involves comparing the forces driving plume ascent and plate subduction. The study does not rely on numerical simulations but instead uses conceptual and physical reasoning to evaluate the balance of forces. The analysis focuses on whether positive or negative buoyancy forces predominate in different scenarios. The study also examines the possibility of symmetric convection, where both forces are balanced. The approach is primarily deductive, based on known principles of convection and buoyancy.
Main Results:
The study suggests that mantle convection is not necessarily force balanced and can be driven by either positive or negative buoyancy forces. Bottom-up convection is driven by plume ascent, while top-down convection is driven by subduction. The balance of these forces depends on the thermal conditions at the top and bottom boundaries of the mantle. The study finds that convection can be symmetric when plume ascent and subduction are balanced. However, the study does not provide definitive evidence for whether convection is dominantly top-down, bottom-up, or time-dependent. The findings indicate that the dominant mode of convection may vary over time depending on boundary conditions. The study also highlights the importance of the core-mantle and lithosphere-asthenosphere boundaries in determining the direction of convection.
Conclusions:
The study concludes that mantle convection is not necessarily force balanced and can be driven by either positive or negative buoyancy forces. The authors suggest that convection can be symmetric when plume ascent and subduction are balanced. However, the study does not provide definitive evidence for whether convection is dominantly top-down, bottom-up, or time-dependent. The findings indicate that the dominant mode of convection may vary over time depending on boundary conditions. The study emphasizes the importance of the core-mantle and lithosphere-asthenosphere boundaries in determining the direction of convection. The authors propose that further research is needed to clarify the mechanisms governing mantle convection and how they evolve over time. The study does not make claims about the necessity of any specific mechanism but highlights the variability of convection based on boundary conditions.
Frequently Asked Questions
Mantle convection is driven by buoyancy forces, which can be either positive (bottom-up) or negative (top-down), depending on thermal conditions at boundary layers.
These boundaries determine the thermal conditions that influence whether convection is driven by plume ascent or plate subduction.
Convection does not require force balance because buoyancy forces can be imbalanced depending on boundary conditions and thermal gradients.
Symmetric convection occurs when plume ascent and subduction forces are balanced, potentially stabilizing mantle dynamics.
The study evaluates thermal gradients and buoyancy forces at the core-mantle and lithosphere-asthenosphere boundaries.
The authors suggest that convection modes may vary over time depending on boundary conditions, but they do not declare this as a necessity.
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