Lights and shadows on the resonant modes of the Earth rotation axis
- Autores
- Bizouard, C.; Dehant, V.; Folgueira, M.
- Año de publicación
- 2025
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- Resonant free modes are of primary important for understanding the terrestrial and celestial oscillations of the rotation axis of a non-rigid Earth. In this talk we present the state of the art of their observation and modeling. We show how mass transports taking place in the hydro-atmospheric layer allows to reconstruct Chandler wobble from the 1950’s, and account in particular for its minimum observed since the 2020. In contrast, the irregularities of the free core nutation remains largely unexplained. Until now, diurnal circulation in the atmosphere and oceans seems to have been powerless, and we shall give the last results in this respect. Finally we shall explore the existence of a supplementary polar motion resonance caused by the inner core.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
Free rotational modes
Chandler wobble
Free core nutation - 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:10915/192034
Ver los metadatos del registro completo
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Lights and shadows on the resonant modes of the Earth rotation axisBizouard, C.Dehant, V.Folgueira, M.Ciencias AstronómicasFree rotational modesChandler wobbleFree core nutationResonant free modes are of primary important for understanding the terrestrial and celestial oscillations of the rotation axis of a non-rigid Earth. In this talk we present the state of the art of their observation and modeling. We show how mass transports taking place in the hydro-atmospheric layer allows to reconstruct Chandler wobble from the 1950’s, and account in particular for its minimum observed since the 2020. In contrast, the irregularities of the free core nutation remains largely unexplained. Until now, diurnal circulation in the atmosphere and oceans seems to have been powerless, and we shall give the last results in this respect. Finally we shall explore the existence of a supplementary polar motion resonance caused by the inner core.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/10915/192034enginfo: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:UNLP2026-03-26T09:21:46Zoai:sedici.unlp.edu.ar:10915/192034Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292026-03-26 09:21:46.949SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
Lights and shadows on the resonant modes of the Earth rotation axis |
| title |
Lights and shadows on the resonant modes of the Earth rotation axis |
| spellingShingle |
Lights and shadows on the resonant modes of the Earth rotation axis Bizouard, C. Ciencias Astronómicas Free rotational modes Chandler wobble Free core nutation |
| title_short |
Lights and shadows on the resonant modes of the Earth rotation axis |
| title_full |
Lights and shadows on the resonant modes of the Earth rotation axis |
| title_fullStr |
Lights and shadows on the resonant modes of the Earth rotation axis |
| title_full_unstemmed |
Lights and shadows on the resonant modes of the Earth rotation axis |
| title_sort |
Lights and shadows on the resonant modes of the Earth rotation axis |
| dc.creator.none.fl_str_mv |
Bizouard, C. Dehant, V. Folgueira, M. |
| author |
Bizouard, C. |
| author_facet |
Bizouard, C. Dehant, V. Folgueira, M. |
| author_role |
author |
| author2 |
Dehant, V. Folgueira, M. |
| author2_role |
author author |
| dc.subject.none.fl_str_mv |
Ciencias Astronómicas Free rotational modes Chandler wobble Free core nutation |
| topic |
Ciencias Astronómicas Free rotational modes Chandler wobble Free core nutation |
| dc.description.none.fl_txt_mv |
Resonant free modes are of primary important for understanding the terrestrial and celestial oscillations of the rotation axis of a non-rigid Earth. In this talk we present the state of the art of their observation and modeling. We show how mass transports taking place in the hydro-atmospheric layer allows to reconstruct Chandler wobble from the 1950’s, and account in particular for its minimum observed since the 2020. In contrast, the irregularities of the free core nutation remains largely unexplained. Until now, diurnal circulation in the atmosphere and oceans seems to have been powerless, and we shall give the last results in this respect. Finally we shall explore the existence of a supplementary polar motion resonance caused by the inner core. Facultad de Ciencias Astronómicas y Geofísicas |
| description |
Resonant free modes are of primary important for understanding the terrestrial and celestial oscillations of the rotation axis of a non-rigid Earth. In this talk we present the state of the art of their observation and modeling. We show how mass transports taking place in the hydro-atmospheric layer allows to reconstruct Chandler wobble from the 1950’s, and account in particular for its minimum observed since the 2020. In contrast, the irregularities of the free core nutation remains largely unexplained. Until now, diurnal circulation in the atmosphere and oceans seems to have been powerless, and we shall give the last results in this respect. Finally we shall explore the existence of a supplementary polar motion resonance caused by the inner core. |
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2025 |
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2025-08 |
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eng |
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