The time-dependent behaviour of a spinning disc on a rotating planet: A model for geophysical vortex motion
作者:
N.Robb McDonald,
期刊:
Geophysical & Astrophysical Fluid Dynamics
(Taylor Available online 1998)
卷期:
Volume 87,
issue 3-4
页码: 253-272
ISSN:0309-1929
年代: 1998
DOI:10.1080/03091929808221149
出版商: Taylor & Francis Group
关键词: Geophysical vortices;spinning disc;trajectories
数据来源: Taylor
摘要:
A recent theory of Nycander (1996) establishing the analogy between the steady westward drift of geophysical vortices and the precession of a rigid-body (in particular a disc spinning about its symmetry axis) is rederived within a Lagrangian framework. This formulation allows the time-dependent properties (e.g., trajectory, spinetc.) of the rigidbody, represented by three coupled ODEs, to be studied. Numerical results for a variety of initial zonal velocities and latitudes are presented. Typically the trajectory consists of a mean westward precession coupled with periodic behaviour which, in the terminology of rigid-body dynamics, is known as nutation. In the limit that β-plane physics are appropriate, it is shown that the nutation is exactly analogous to harmonic inertial oscillations at the local Coriolis frequency.
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