Glacial isostatic adjustment: physical models and observational constraints

By far the most prescient insights into the interior structure of the planet have been provided on the basis of elastic wave seismology. Analysis of the travel times of shear or compression wave phases excited by individual earthquakes, or through analysis of the elastic gravitational free oscillati...

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Main Authors: Peltier, W. Richard, Wu, Patrick Pak-Cheuk, Argus, Donald F., Li, Tanghua, Velay-Vitow, Jesse
Other Authors: Earth Observatory of Singapore
Format: Article
Language:English
Published: 2023
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Online Access:https://hdl.handle.net/10356/168866
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Institution: Nanyang Technological University
Language: English
id sg-ntu-dr.10356-168866
record_format dspace
institution Nanyang Technological University
building NTU Library
continent Asia
country Singapore
Singapore
content_provider NTU Library
collection DR-NTU
language English
topic Science::Geology
Glacial Isostatic Adjustment
Review
spellingShingle Science::Geology
Glacial Isostatic Adjustment
Review
Peltier, W. Richard
Wu, Patrick Pak-Cheuk
Argus, Donald F.
Li, Tanghua
Velay-Vitow, Jesse
Glacial isostatic adjustment: physical models and observational constraints
description By far the most prescient insights into the interior structure of the planet have been provided on the basis of elastic wave seismology. Analysis of the travel times of shear or compression wave phases excited by individual earthquakes, or through analysis of the elastic gravitational free oscillations that individual earthquakes of sufficiently large magnitude may excite, has been the central focus of Earth physics research for more than a century. Unfortunately, data provide no information that is directly relevant to understanding the solid state ‘flow’ of the polycrystalline outer ‘mantle’ shell of the planet that is involved in the thermally driven convective circulation that is responsible for powering the ‘drift’ of the continents and which controls the rate of planetary cooling on long timescales. For this reason, there has been an increasing focus on the understanding of physical phenomenology that is unambiguously associated with mantle flow processes that are distinct from those directly associated with the convective circulation itself. This paper reviews the past many decades of work that has been invested in understanding the most important of such processes, namely that which has come to be referred to as ‘glacial isostatic adjustment’ (GIA). This process concerns the response of the planet to the loading and unloading of the high latitude continents by the massive accumulations of glacial ice that have occurred with almost metronomic regularity over the most recent million years of Earth history. Forced by the impact of gravitational n-body effects on the geometry of Earth’s orbit around the Sun through the impact upon the terrestrial regime of received solar insolation, these surface mass loads on the continents have left indelible records of their occurrence in the ‘Earth system’ consisting of the oceans, continents, and the great polar ice sheets on Greenland and Antarctica themselves. Although this ice-age phenomenology has been clearly recognized since early in the last century, it was for over 50 years considered to be no more than an interesting curiosity, the understanding of which remained on the periphery of the theoretical physics of the Earth. This was the case in part because no globally applicable theory was available that could be applied to rigorously interpret the observations. Equally important to understanding the scientific lethargy that held back the understanding of this phenomenon involving mantle flow processes was the lack of appreciation of the wide range of observations that were in fact related to GIA physics. This paper is devoted to a review of the global theories of the GIA process that have since been developed as a means of interpreting the extensive variety of observations that are now recognized as being involved in the response of the planet to the loading and unloading of its surface by glacial ice. The paper will also provide examples of the further analyses of Earth physics and climate related processes that applications of the modern theoretical structures have enabled.
author2 Earth Observatory of Singapore
author_facet Earth Observatory of Singapore
Peltier, W. Richard
Wu, Patrick Pak-Cheuk
Argus, Donald F.
Li, Tanghua
Velay-Vitow, Jesse
format Article
author Peltier, W. Richard
Wu, Patrick Pak-Cheuk
Argus, Donald F.
Li, Tanghua
Velay-Vitow, Jesse
author_sort Peltier, W. Richard
title Glacial isostatic adjustment: physical models and observational constraints
title_short Glacial isostatic adjustment: physical models and observational constraints
title_full Glacial isostatic adjustment: physical models and observational constraints
title_fullStr Glacial isostatic adjustment: physical models and observational constraints
title_full_unstemmed Glacial isostatic adjustment: physical models and observational constraints
title_sort glacial isostatic adjustment: physical models and observational constraints
publishDate 2023
url https://hdl.handle.net/10356/168866
_version_ 1772828239067086848
spelling sg-ntu-dr.10356-1688662023-06-27T15:36:33Z Glacial isostatic adjustment: physical models and observational constraints Peltier, W. Richard Wu, Patrick Pak-Cheuk Argus, Donald F. Li, Tanghua Velay-Vitow, Jesse Earth Observatory of Singapore Science::Geology Glacial Isostatic Adjustment Review By far the most prescient insights into the interior structure of the planet have been provided on the basis of elastic wave seismology. Analysis of the travel times of shear or compression wave phases excited by individual earthquakes, or through analysis of the elastic gravitational free oscillations that individual earthquakes of sufficiently large magnitude may excite, has been the central focus of Earth physics research for more than a century. Unfortunately, data provide no information that is directly relevant to understanding the solid state ‘flow’ of the polycrystalline outer ‘mantle’ shell of the planet that is involved in the thermally driven convective circulation that is responsible for powering the ‘drift’ of the continents and which controls the rate of planetary cooling on long timescales. For this reason, there has been an increasing focus on the understanding of physical phenomenology that is unambiguously associated with mantle flow processes that are distinct from those directly associated with the convective circulation itself. This paper reviews the past many decades of work that has been invested in understanding the most important of such processes, namely that which has come to be referred to as ‘glacial isostatic adjustment’ (GIA). This process concerns the response of the planet to the loading and unloading of the high latitude continents by the massive accumulations of glacial ice that have occurred with almost metronomic regularity over the most recent million years of Earth history. Forced by the impact of gravitational n-body effects on the geometry of Earth’s orbit around the Sun through the impact upon the terrestrial regime of received solar insolation, these surface mass loads on the continents have left indelible records of their occurrence in the ‘Earth system’ consisting of the oceans, continents, and the great polar ice sheets on Greenland and Antarctica themselves. Although this ice-age phenomenology has been clearly recognized since early in the last century, it was for over 50 years considered to be no more than an interesting curiosity, the understanding of which remained on the periphery of the theoretical physics of the Earth. This was the case in part because no globally applicable theory was available that could be applied to rigorously interpret the observations. Equally important to understanding the scientific lethargy that held back the understanding of this phenomenon involving mantle flow processes was the lack of appreciation of the wide range of observations that were in fact related to GIA physics. This paper is devoted to a review of the global theories of the GIA process that have since been developed as a means of interpreting the extensive variety of observations that are now recognized as being involved in the response of the planet to the loading and unloading of its surface by glacial ice. The paper will also provide examples of the further analyses of Earth physics and climate related processes that applications of the modern theoretical structures have enabled. Ministry of Education (MOE) National Research Foundation (NRF) Submitted/Accepted version Tanghua Li is supported by the Singapore Ministry of Education Academic Research Fund MOE2019-T3- 1-004 and MOE2018-T2-1-030, the National Research Foundation Singapore, and the Singapore Ministry of Education, under the Research Centers of Excellence initiative. This work comprises Earth Observatory of Singapore Contribution No. 428. Jesse Velay-Vitow is supported by NSERC Grant CGSD3—547034—2020 as well as by the Walter C Sumner Mmeorial Foundation. 2023-06-21T06:41:56Z 2023-06-21T06:41:56Z 2022 Journal Article Peltier, W. R., Wu, P. P., Argus, D. F., Li, T. & Velay-Vitow, J. (2022). Glacial isostatic adjustment: physical models and observational constraints. Reports On Progress in Physics, 85(9), 096801-. https://dx.doi.org/10.1088/1361-6633/ac805b 0034-4885 https://hdl.handle.net/10356/168866 10.1088/1361-6633/ac805b 85 2-s2.0-85138460242 9 85 096801 en MOE2019-T3-1-004 MOE-T2EP50120-0007 Reports on Progress in Physics © 2022 IOP Publishing Ltd. All rights reserved. This is an author-created, un-copyedited version of an article accepted for publication in Reports on Progress in Physics. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The definitive publisher authenticated version is available online at https://doi.org/10.1088/1361-6633/ac805b. application/pdf