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Evolving mantle convection from bottom up to top down

When it comes to convection, what goes up must come down. Or is it, what goes down must come up? The truth is it depends. Although convection must be mass balanced, there is no reason that it must be force balanced: the positive and negative buoyancy forces driving convection up and down, respective...

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Detalles Bibliográficos
Autores principales: Mitchell, Ross N., Brown, Michael, Gernon, Thomas M., Spencer, Christopher J.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Elsevier 2022
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9508149/
https://www.ncbi.nlm.nih.gov/pubmed/36164640
http://dx.doi.org/10.1016/j.xinn.2022.100309
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author Mitchell, Ross N.
Brown, Michael
Gernon, Thomas M.
Spencer, Christopher J.
author_facet Mitchell, Ross N.
Brown, Michael
Gernon, Thomas M.
Spencer, Christopher J.
author_sort Mitchell, Ross N.
collection PubMed
description When it comes to convection, what goes up must come down. Or is it, what goes down must come up? The truth is it depends. Although convection must be mass balanced, there is no reason that it must be force balanced: the positive and negative buoyancy forces driving convection up and down, respectively, do not necessarily need to be balanced. The balance, or imbalance, all depends on the top and bottom boundary layers. Thus, convection in Earth’s mantle depends on the temperature differences across the core–mantle boundary below and the lithosphere–asthenosphere boundary above. Convective asymmetry predominated by positive buoyancy, or bottom-up convection, would be driven by plume ascent, whereas if it were predominated by negative buoyancy, or top-down convection, it would be driven by plate subduction. Symmetric convection would balance plume ascent and plate subduction. Is mantle convection on Earth balanced, dominantly top down or bottom up, or time dependent?
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spelling pubmed-95081492022-09-25 Evolving mantle convection from bottom up to top down Mitchell, Ross N. Brown, Michael Gernon, Thomas M. Spencer, Christopher J. Innovation (Camb) Commentary When it comes to convection, what goes up must come down. Or is it, what goes down must come up? The truth is it depends. Although convection must be mass balanced, there is no reason that it must be force balanced: the positive and negative buoyancy forces driving convection up and down, respectively, do not necessarily need to be balanced. The balance, or imbalance, all depends on the top and bottom boundary layers. Thus, convection in Earth’s mantle depends on the temperature differences across the core–mantle boundary below and the lithosphere–asthenosphere boundary above. Convective asymmetry predominated by positive buoyancy, or bottom-up convection, would be driven by plume ascent, whereas if it were predominated by negative buoyancy, or top-down convection, it would be driven by plate subduction. Symmetric convection would balance plume ascent and plate subduction. Is mantle convection on Earth balanced, dominantly top down or bottom up, or time dependent? Elsevier 2022-09-06 /pmc/articles/PMC9508149/ /pubmed/36164640 http://dx.doi.org/10.1016/j.xinn.2022.100309 Text en © 2022 The Author(s) https://creativecommons.org/licenses/by-nc-nd/4.0/This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/).
spellingShingle Commentary
Mitchell, Ross N.
Brown, Michael
Gernon, Thomas M.
Spencer, Christopher J.
Evolving mantle convection from bottom up to top down
title Evolving mantle convection from bottom up to top down
title_full Evolving mantle convection from bottom up to top down
title_fullStr Evolving mantle convection from bottom up to top down
title_full_unstemmed Evolving mantle convection from bottom up to top down
title_short Evolving mantle convection from bottom up to top down
title_sort evolving mantle convection from bottom up to top down
topic Commentary
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9508149/
https://www.ncbi.nlm.nih.gov/pubmed/36164640
http://dx.doi.org/10.1016/j.xinn.2022.100309
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