Glacial isostatic adjustment on a rotating earth

We extend and complete previous work to compute the influence of perturbations to the rotation vector on a suite of observables associated with glacial isostatic adjustment (GIA). We emphasize observables relevant to present and future geodetic missions (for example, present-day 3-D crustal motions,...

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Published in:Geophysical Journal International
Main Authors: Mitrovica, Jerry X., Milne, Glenn A., Davis, James L.
Format: Text
Language:English
Published: Oxford University Press 2001
Subjects:
Online Access:http://gji.oxfordjournals.org/cgi/content/short/147/3/562
https://doi.org/10.1046/j.1365-246x.2001.01550.x
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spelling fthighwire:oai:open-archive.highwire.org:gji:147/3/562 2023-05-15T16:29:51+02:00 Glacial isostatic adjustment on a rotating earth Mitrovica, Jerry X. Milne, Glenn A. Davis, James L. 2001-12-01 00:00:00.0 text/html http://gji.oxfordjournals.org/cgi/content/short/147/3/562 https://doi.org/10.1046/j.1365-246x.2001.01550.x en eng Oxford University Press http://gji.oxfordjournals.org/cgi/content/short/147/3/562 http://dx.doi.org/10.1046/j.1365-246x.2001.01550.x Copyright (C) 2001, Oxford University Press Articles TEXT 2001 fthighwire https://doi.org/10.1046/j.1365-246x.2001.01550.x 2013-05-27T12:28:30Z We extend and complete previous work to compute the influence of perturbations to the rotation vector on a suite of observables associated with glacial isostatic adjustment (GIA). We emphasize observables relevant to present and future geodetic missions (for example, present-day 3-D crustal motions, relative sea-level change and geoid or absolute sea-level variations). Our calculations adopt spherically symmetric, self-gravitating, Maxwell viscoelastic earth models while incorporating realistic mass (ice plus ocean) load and rotation variations. The predicted rotation-induced signals are dominated by the influence of true polar wander (TPW). The spatial geometry of the TPW-induced relative sea level, geoid and radial velocity fields is primarily that of a degree two, order one surface spherical harmonic. The spatial variation of the horizontal velocity vectors is given by the gradient of this harmonic. The peak radial and horizontal velocities are of the order of 0.5 mm yr−1; however, we show that this value is sensitive to the adopted profile of mantle viscosity. We also demonstrate that an accurate prediction of TPW-induced sea level and 3-D crustal deformation rates requires that a realistic number of glacial cycles be incorporated into the ice load history. We conclude that geodetic observations of the GIA process should be analysed using a GIA theory valid for a rotating planet. Finally, we also consider variations in rotation driven by simple present-day polar melting scenarios and predict the influence of these variations on a suite of geophysical observables. We find that the rotational feedback associated with Greenland melting is capable of significantly perturbing both relative and absolute sea-level variations. Text Greenland HighWire Press (Stanford University) Greenland Geophysical Journal International 147 3 562 578
institution Open Polar
collection HighWire Press (Stanford University)
op_collection_id fthighwire
language English
topic Articles
spellingShingle Articles
Mitrovica, Jerry X.
Milne, Glenn A.
Davis, James L.
Glacial isostatic adjustment on a rotating earth
topic_facet Articles
description We extend and complete previous work to compute the influence of perturbations to the rotation vector on a suite of observables associated with glacial isostatic adjustment (GIA). We emphasize observables relevant to present and future geodetic missions (for example, present-day 3-D crustal motions, relative sea-level change and geoid or absolute sea-level variations). Our calculations adopt spherically symmetric, self-gravitating, Maxwell viscoelastic earth models while incorporating realistic mass (ice plus ocean) load and rotation variations. The predicted rotation-induced signals are dominated by the influence of true polar wander (TPW). The spatial geometry of the TPW-induced relative sea level, geoid and radial velocity fields is primarily that of a degree two, order one surface spherical harmonic. The spatial variation of the horizontal velocity vectors is given by the gradient of this harmonic. The peak radial and horizontal velocities are of the order of 0.5 mm yr−1; however, we show that this value is sensitive to the adopted profile of mantle viscosity. We also demonstrate that an accurate prediction of TPW-induced sea level and 3-D crustal deformation rates requires that a realistic number of glacial cycles be incorporated into the ice load history. We conclude that geodetic observations of the GIA process should be analysed using a GIA theory valid for a rotating planet. Finally, we also consider variations in rotation driven by simple present-day polar melting scenarios and predict the influence of these variations on a suite of geophysical observables. We find that the rotational feedback associated with Greenland melting is capable of significantly perturbing both relative and absolute sea-level variations.
format Text
author Mitrovica, Jerry X.
Milne, Glenn A.
Davis, James L.
author_facet Mitrovica, Jerry X.
Milne, Glenn A.
Davis, James L.
author_sort Mitrovica, Jerry X.
title Glacial isostatic adjustment on a rotating earth
title_short Glacial isostatic adjustment on a rotating earth
title_full Glacial isostatic adjustment on a rotating earth
title_fullStr Glacial isostatic adjustment on a rotating earth
title_full_unstemmed Glacial isostatic adjustment on a rotating earth
title_sort glacial isostatic adjustment on a rotating earth
publisher Oxford University Press
publishDate 2001
url http://gji.oxfordjournals.org/cgi/content/short/147/3/562
https://doi.org/10.1046/j.1365-246x.2001.01550.x
geographic Greenland
geographic_facet Greenland
genre Greenland
genre_facet Greenland
op_relation http://gji.oxfordjournals.org/cgi/content/short/147/3/562
http://dx.doi.org/10.1046/j.1365-246x.2001.01550.x
op_rights Copyright (C) 2001, Oxford University Press
op_doi https://doi.org/10.1046/j.1365-246x.2001.01550.x
container_title Geophysical Journal International
container_volume 147
container_issue 3
container_start_page 562
op_container_end_page 578
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