Abstract
The steady-state Chandler wobble of the Earth’s pole is investigated for various choices of the pole tide model. The aim of the work is to estimate the parameters of the stationary Chandler wobble. The steady motion of the Earth’s pole is considered taking into account the pole tide, which depends both on the position and on the speed of the pole. The Chandler motion of the Earth’s pole is studied on the basis of the Euler-Liouville equations with a variable tensor of inertia. It is shown that both the choice of the pole tide model and the method of estimating the parameters of the chosen model significantly affect the parameters of the steady oscillatory process of the earth’s pole and the amplitude of the necessary disturbance to excite the observed Chandler wobble.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
