Interannual changes in length-of-day driven by a hydromagnetic core waves inside the fluid outer core

Autores
Duan, P.; Huang, C.
Año de publicación
2025
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
Variations in Earth rotation rate defined by length-of-day (LOD) on the intradecadal scales present two primary period (i.e., 6yr and 8.6yr) oscillations, the physical mechanisms for them are still uncertain. Based on the core surface flow data inferred from modern satellite magnetic observations for 1999 to the present, we calculate the electromagnetic torque exerting on the mantle from core flow motions and show that the torque also presents the same two period oscillations, providing new evidence to show that intradecadal LOD oscillations are driven by the core motions. Using the purely geostrophic core flow model described in the framework of torsional waves, this work shows that the predicted 6yr LOD result coincides well with the observation, while the observed 8.6yr LOD oscillation cannot be satisfactorily explained by this model due to the existing phase difference with ~ 2 years. This work further develops the novel model of LOD changes attributed to the quasi-geostrophic magneto-Coriolis (QG-MC) waves, suggesting that the QG-MC wave modes with cylindrical radial wave number ~4.8 and quality factor Q ~ 16 can provide a nice explanation for the 8.6yr LOD oscillation (including both amplitude and phase) and providing a new approach to infer the information of core dynamics via LOD changes.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Ciencias Astronómicas
Length-of-day (LOD) variations
Core-mantle coupling
Magneto-Coriolis waves
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-nd/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/192033

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spelling Interannual changes in length-of-day driven by a hydromagnetic core waves inside the fluid outer coreDuan, P.Huang, C.Ciencias AstronómicasLength-of-day (LOD) variationsCore-mantle couplingMagneto-Coriolis wavesVariations in Earth rotation rate defined by length-of-day (LOD) on the intradecadal scales present two primary period (i.e., 6yr and 8.6yr) oscillations, the physical mechanisms for them are still uncertain. Based on the core surface flow data inferred from modern satellite magnetic observations for 1999 to the present, we calculate the electromagnetic torque exerting on the mantle from core flow motions and show that the torque also presents the same two period oscillations, providing new evidence to show that intradecadal LOD oscillations are driven by the core motions. Using the purely geostrophic core flow model described in the framework of torsional waves, this work shows that the predicted 6yr LOD result coincides well with the observation, while the observed 8.6yr LOD oscillation cannot be satisfactorily explained by this model due to the existing phase difference with ~ 2 years. This work further develops the novel model of LOD changes attributed to the quasi-geostrophic magneto-Coriolis (QG-MC) waves, suggesting that the QG-MC wave modes with cylindrical radial wave number ~4.8 and quality factor Q ~ 16 can provide a nice explanation for the 8.6yr LOD oscillation (including both amplitude and phase) and providing a new approach to infer the information of core dynamics via LOD changes.Facultad de Ciencias Astronómicas y Geofísicas2025-08info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionResumenhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/192033enginfo:eu-repo/semantics/reference/url/https://sedici.unlp.edu.ar/handle/10915/190232info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-nd/4.0/Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2026-05-13T12:59:23Zoai:sedici.unlp.edu.ar:10915/192033Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292026-05-13 12:59:24.213SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Interannual changes in length-of-day driven by a hydromagnetic core waves inside the fluid outer core
title Interannual changes in length-of-day driven by a hydromagnetic core waves inside the fluid outer core
spellingShingle Interannual changes in length-of-day driven by a hydromagnetic core waves inside the fluid outer core
Duan, P.
Ciencias Astronómicas
Length-of-day (LOD) variations
Core-mantle coupling
Magneto-Coriolis waves
title_short Interannual changes in length-of-day driven by a hydromagnetic core waves inside the fluid outer core
title_full Interannual changes in length-of-day driven by a hydromagnetic core waves inside the fluid outer core
title_fullStr Interannual changes in length-of-day driven by a hydromagnetic core waves inside the fluid outer core
title_full_unstemmed Interannual changes in length-of-day driven by a hydromagnetic core waves inside the fluid outer core
title_sort Interannual changes in length-of-day driven by a hydromagnetic core waves inside the fluid outer core
dc.creator.none.fl_str_mv Duan, P.
Huang, C.
author Duan, P.
author_facet Duan, P.
Huang, C.
author_role author
author2 Huang, C.
author2_role author
dc.subject.none.fl_str_mv Ciencias Astronómicas
Length-of-day (LOD) variations
Core-mantle coupling
Magneto-Coriolis waves
topic Ciencias Astronómicas
Length-of-day (LOD) variations
Core-mantle coupling
Magneto-Coriolis waves
dc.description.none.fl_txt_mv Variations in Earth rotation rate defined by length-of-day (LOD) on the intradecadal scales present two primary period (i.e., 6yr and 8.6yr) oscillations, the physical mechanisms for them are still uncertain. Based on the core surface flow data inferred from modern satellite magnetic observations for 1999 to the present, we calculate the electromagnetic torque exerting on the mantle from core flow motions and show that the torque also presents the same two period oscillations, providing new evidence to show that intradecadal LOD oscillations are driven by the core motions. Using the purely geostrophic core flow model described in the framework of torsional waves, this work shows that the predicted 6yr LOD result coincides well with the observation, while the observed 8.6yr LOD oscillation cannot be satisfactorily explained by this model due to the existing phase difference with ~ 2 years. This work further develops the novel model of LOD changes attributed to the quasi-geostrophic magneto-Coriolis (QG-MC) waves, suggesting that the QG-MC wave modes with cylindrical radial wave number ~4.8 and quality factor Q ~ 16 can provide a nice explanation for the 8.6yr LOD oscillation (including both amplitude and phase) and providing a new approach to infer the information of core dynamics via LOD changes.
Facultad de Ciencias Astronómicas y Geofísicas
description Variations in Earth rotation rate defined by length-of-day (LOD) on the intradecadal scales present two primary period (i.e., 6yr and 8.6yr) oscillations, the physical mechanisms for them are still uncertain. Based on the core surface flow data inferred from modern satellite magnetic observations for 1999 to the present, we calculate the electromagnetic torque exerting on the mantle from core flow motions and show that the torque also presents the same two period oscillations, providing new evidence to show that intradecadal LOD oscillations are driven by the core motions. Using the purely geostrophic core flow model described in the framework of torsional waves, this work shows that the predicted 6yr LOD result coincides well with the observation, while the observed 8.6yr LOD oscillation cannot be satisfactorily explained by this model due to the existing phase difference with ~ 2 years. This work further develops the novel model of LOD changes attributed to the quasi-geostrophic magneto-Coriolis (QG-MC) waves, suggesting that the QG-MC wave modes with cylindrical radial wave number ~4.8 and quality factor Q ~ 16 can provide a nice explanation for the 8.6yr LOD oscillation (including both amplitude and phase) and providing a new approach to infer the information of core dynamics via LOD changes.
publishDate 2025
dc.date.none.fl_str_mv 2025-08
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Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)
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