A coupled core-mantle evolution: review and future prospects

Abstract In this review, I provide the current status and future prospects for the coupled core-mantle evolution and specifically summarize the constraints arising from geomagnetism and paleomagnetism on the long-term secular variations of the geomagnetic field. The heat flow across the core-mantle...

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Main Author: Takashi Nakagawa
Format: Article
Language:English
Published: SpringerOpen 2020-10-01
Series:Progress in Earth and Planetary Science
Subjects:
Online Access:http://link.springer.com/article/10.1186/s40645-020-00374-8
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author Takashi Nakagawa
author_facet Takashi Nakagawa
author_sort Takashi Nakagawa
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description Abstract In this review, I provide the current status and future prospects for the coupled core-mantle evolution and specifically summarize the constraints arising from geomagnetism and paleomagnetism on the long-term secular variations of the geomagnetic field. The heat flow across the core-mantle boundary (CMB) is essential for determining the best-fit scenario that explains the observational data of geomagnetic secular variations (e.g., onset timing of the inner core growth, geomagnetic polarity reversals, and westward drift) and should include the various origins of the heterogeneous structures in the deep mantle that have affected the heat transfer across the core-mantle boundary for billions of years. The coupled core-mantle evolution model can potentially explain the onset timing of the inner core and its influence on the long-term geomagnetic secular variations, but it is still controversial among modeling approaches on the core energetics because the paleomagnetic data contains various uncertainties. Additionally, with the coupled core-mantle evolution model in geodynamo simulations, the frequency of the geomagnetic polarity reversals can be explained with the time variations of the heat flow across the CMB. Additionally, the effects of the stable region in the outermost outer core to the magnetic evolution are also crucial but there would be still uncertain for their feasibility. However, despite this progress in understanding the observational data for geomagnetic secular variations, there are several unresolved issues that should be addressed in future investigations: (1) initial conditions—starting with the solidification of the global magma ocean with the onset timing of plate tectonics and geodynamo actions and (2) planetary habitability—how the dynamics of the Earth’s deep interior affects the long-term surface environment change that has been maintained in the Earth’s multisphere coupled system.
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spelling doaj.art-c557d650d39c4d6e8d1553eb54389e7e2022-12-21T18:59:09ZengSpringerOpenProgress in Earth and Planetary Science2197-42842020-10-017111710.1186/s40645-020-00374-8A coupled core-mantle evolution: review and future prospectsTakashi Nakagawa0Division of Earth and Planetary Sciences, The University of Hong KongAbstract In this review, I provide the current status and future prospects for the coupled core-mantle evolution and specifically summarize the constraints arising from geomagnetism and paleomagnetism on the long-term secular variations of the geomagnetic field. The heat flow across the core-mantle boundary (CMB) is essential for determining the best-fit scenario that explains the observational data of geomagnetic secular variations (e.g., onset timing of the inner core growth, geomagnetic polarity reversals, and westward drift) and should include the various origins of the heterogeneous structures in the deep mantle that have affected the heat transfer across the core-mantle boundary for billions of years. The coupled core-mantle evolution model can potentially explain the onset timing of the inner core and its influence on the long-term geomagnetic secular variations, but it is still controversial among modeling approaches on the core energetics because the paleomagnetic data contains various uncertainties. Additionally, with the coupled core-mantle evolution model in geodynamo simulations, the frequency of the geomagnetic polarity reversals can be explained with the time variations of the heat flow across the CMB. Additionally, the effects of the stable region in the outermost outer core to the magnetic evolution are also crucial but there would be still uncertain for their feasibility. However, despite this progress in understanding the observational data for geomagnetic secular variations, there are several unresolved issues that should be addressed in future investigations: (1) initial conditions—starting with the solidification of the global magma ocean with the onset timing of plate tectonics and geodynamo actions and (2) planetary habitability—how the dynamics of the Earth’s deep interior affects the long-term surface environment change that has been maintained in the Earth’s multisphere coupled system.http://link.springer.com/article/10.1186/s40645-020-00374-8Geomagnetic fieldEarth’s coreDeep mantleLong-term evolution
spellingShingle Takashi Nakagawa
A coupled core-mantle evolution: review and future prospects
Progress in Earth and Planetary Science
Geomagnetic field
Earth’s core
Deep mantle
Long-term evolution
title A coupled core-mantle evolution: review and future prospects
title_full A coupled core-mantle evolution: review and future prospects
title_fullStr A coupled core-mantle evolution: review and future prospects
title_full_unstemmed A coupled core-mantle evolution: review and future prospects
title_short A coupled core-mantle evolution: review and future prospects
title_sort coupled core mantle evolution review and future prospects
topic Geomagnetic field
Earth’s core
Deep mantle
Long-term evolution
url http://link.springer.com/article/10.1186/s40645-020-00374-8
work_keys_str_mv AT takashinakagawa acoupledcoremantleevolutionreviewandfutureprospects
AT takashinakagawa coupledcoremantleevolutionreviewandfutureprospects