2026-06-07T17:24:50Zhttps://docta.ucm.es/rest/oai/requestoai:docta.ucm.es:20.500.14352/572962024-07-17T14:39:57Zcom_20.500.14352_14col_20.500.14352_15
Docta Complutense
author
Folgueira López, Marta
author
Souchay, J.
author
Kinoshita, Hiroshi
2023-06-20T16:52:33Z
2023-06-20T16:52:33Z
1998
0923-2958
10.1023/A:1008298122976
https://hdl.handle.net/20.500.14352/57296
https//doi.org/10.1023/A:1008298122976
http://www.springerlink.com/content/p004831g80371110/fulltext.pdf
In this paper, we calculate the coefficients of the nutation for a rigid Earth model due to the C-3m and S-3m (m not equal 0) harmonics of the geopotential, starting from the Hamiltonian theory as developped by Kinoshita (1977). We show that these coefficients are far from bring negligible as given the level of truncation of 0.1 mu as which is necessary in the reconstruction of the tables of nutation, and also that their value is very close to that given by Bretagnon st al. (1997).
eng
Effects on the nutation of the non-zonal harmonics of third degree
journal article
URL
https://docta.ucm.es/bitstreams/acd6c073-1489-4bae-90da-811b29584ba7/download
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9b203d1ae24148a1f43f0a15c1fae1f7
149358
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13.pdf