Reconstruction of prograde and retrograde Chandler excitation - Université Pierre et Marie Curie Accéder directement au contenu
Article Dans Une Revue Journal of Inverse and Ill-posed Problems Année : 2015

Reconstruction of prograde and retrograde Chandler excitation

Résumé

Observed polar motion consists of uniform circular motions at both positive (prograde) and negative (retrograde) frequencies. Generalized Euler–Liouville equations of Bizouard, taking into account Earth's triaxiality and asymmetry of the ocean tide, show that the corresponding retrograde and prograde circular excitations are coupled at any frequency. In this work, we reconstructed the polar motion excitation in the Chandler band (prograde and retrograde). Then we compared it with geophysical excitation, filtered out in the same way from the series of the Oceanic Angular Momentum (OAM) and Atmospheric Angular Momentum (AAM) for the period 1960–2000. The agreement was found to be better in the prograde band than in the retrograde one.
Fichier non déposé

Dates et versions

hal-03801273 , version 1 (06-10-2022)

Identifiants

  • HAL Id : hal-03801273 , version 1

Citer

Leonid Zotov, Christian Bizouard. Reconstruction of prograde and retrograde Chandler excitation. Journal of Inverse and Ill-posed Problems, 2015, 24 (1). ⟨hal-03801273⟩
4 Consultations
0 Téléchargements

Partager

Gmail Facebook X LinkedIn More