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
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/192033
Ver los metadatos del registro completo
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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 |
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2025-08 |
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eng |
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