Earth Rotation: Measurement of TT-UT, -720 to +1950
- Autores
- Morrison, L.V.; Hohenkerk, C.Y.; Stephenson, F.R.; Zawilski, M.
- Año de publicación
- 2025
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- We present figures and tables of our results for DT=TT-UT in the period -720 to +1950 obtained principally from analyses of historical records of solar eclipses (-720 to +1600) and timings of lunar occultations ( + 1600 to + 1950) [1], These show changes in the Earth’s rate of rotation as measured in changes of the length of the day (lod). There is a long-term deceleration producing an increase in the lod of +1.72 ms cy-1. There are also centennial fluctuations in the lod of amplitude 3 ms. After +1600 the data are precise enough to reveal decade fluctuations of up to an amplitude of 4 ms.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
Delta T
Length of Day
Earth's rotation rate - 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:10915/192193
Ver los metadatos del registro completo
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Earth Rotation: Measurement of TT-UT, -720 to +1950Morrison, L.V.Hohenkerk, C.Y.Stephenson, F.R.Zawilski, M.Ciencias AstronómicasDelta TLength of DayEarth's rotation rateWe present figures and tables of our results for DT=TT-UT in the period -720 to +1950 obtained principally from analyses of historical records of solar eclipses (-720 to +1600) and timings of lunar occultations ( + 1600 to + 1950) [1], These show changes in the Earth’s rate of rotation as measured in changes of the length of the day (lod). There is a long-term deceleration producing an increase in the lod of +1.72 ms cy-1. There are also centennial fluctuations in the lod of amplitude 3 ms. After +1600 the data are precise enough to reveal decade fluctuations of up to an amplitude of 4 ms.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/10915/192193enginfo: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:UNLP2026-04-23T11:55:44Zoai:sedici.unlp.edu.ar:10915/192193Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292026-04-23 11:55:44.96SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
Earth Rotation: Measurement of TT-UT, -720 to +1950 |
| title |
Earth Rotation: Measurement of TT-UT, -720 to +1950 |
| spellingShingle |
Earth Rotation: Measurement of TT-UT, -720 to +1950 Morrison, L.V. Ciencias Astronómicas Delta T Length of Day Earth's rotation rate |
| title_short |
Earth Rotation: Measurement of TT-UT, -720 to +1950 |
| title_full |
Earth Rotation: Measurement of TT-UT, -720 to +1950 |
| title_fullStr |
Earth Rotation: Measurement of TT-UT, -720 to +1950 |
| title_full_unstemmed |
Earth Rotation: Measurement of TT-UT, -720 to +1950 |
| title_sort |
Earth Rotation: Measurement of TT-UT, -720 to +1950 |
| dc.creator.none.fl_str_mv |
Morrison, L.V. Hohenkerk, C.Y. Stephenson, F.R. Zawilski, M. |
| author |
Morrison, L.V. |
| author_facet |
Morrison, L.V. Hohenkerk, C.Y. Stephenson, F.R. Zawilski, M. |
| author_role |
author |
| author2 |
Hohenkerk, C.Y. Stephenson, F.R. Zawilski, M. |
| author2_role |
author author author |
| dc.subject.none.fl_str_mv |
Ciencias Astronómicas Delta T Length of Day Earth's rotation rate |
| topic |
Ciencias Astronómicas Delta T Length of Day Earth's rotation rate |
| dc.description.none.fl_txt_mv |
We present figures and tables of our results for DT=TT-UT in the period -720 to +1950 obtained principally from analyses of historical records of solar eclipses (-720 to +1600) and timings of lunar occultations ( + 1600 to + 1950) [1], These show changes in the Earth’s rate of rotation as measured in changes of the length of the day (lod). There is a long-term deceleration producing an increase in the lod of +1.72 ms cy-1. There are also centennial fluctuations in the lod of amplitude 3 ms. After +1600 the data are precise enough to reveal decade fluctuations of up to an amplitude of 4 ms. Facultad de Ciencias Astronómicas y Geofísicas |
| description |
We present figures and tables of our results for DT=TT-UT in the period -720 to +1950 obtained principally from analyses of historical records of solar eclipses (-720 to +1600) and timings of lunar occultations ( + 1600 to + 1950) [1], These show changes in the Earth’s rate of rotation as measured in changes of the length of the day (lod). There is a long-term deceleration producing an increase in the lod of +1.72 ms cy-1. There are also centennial fluctuations in the lod of amplitude 3 ms. After +1600 the data are precise enough to reveal decade fluctuations of up to an amplitude of 4 ms. |
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2025 |
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2025-08 |
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info:eu-repo/semantics/conferenceObject info:eu-repo/semantics/publishedVersion Resumen http://purl.org/coar/resource_type/c_5794 info:ar-repo/semantics/documentoDeConferencia |
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eng |
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info:eu-repo/semantics/reference/url/https://sedici.unlp.edu.ar/handle/10915/190232 |
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