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Nonlinear resonance and instability of planetary waves and low-frequency variability in the atmosphere

Journal Article · · Journal of the Atmospheric Sciences; (United States)
 [1]
  1. Imperial College, London (United Kingdom)
It is demonstrated in this work that linearly unstable planetary waves can be resonantly excited to finite amplitude in a nonlinear barotropic atmosphere with vorticity forcing and dissipation. In a weakly forced/dissipated atmosphere, it is shown that barotropic instability may provide a dynamic mechanism of transition between different [open quotes]flow regimes.[close quotes] It is suggested that nonlinear resonance and instability of planetary waves, which seem to be common with finite amplitude steady free solutions, may play a role in producing low-frequency variability observed in the real atmosphere. A type of nonlinear free solution with realistically sheared zonal flow is described in spherical geometry, and normal-mode instability analysis is performed to examine its stability. A time-dependent spectral model is employed to demonstrate the resonant excitation and breakdown of unstable planetary waves that results in low-frequency variability. The steady free solution is barotropically unstable to large-scale, low-frequency perturbations. Even though unstable, it can be resonantly excited from many initial conditions by a stationary vorticity forcing that projects onto it. The leading low-frequency oscillation has a period of about 20 days and the model flow hemispherically alternates between an almost zonal flow and a blocking regime, reminiscent of the multiple equilibria found by Charney and DeVore. 25 refs., 37 figs., 1 tab.
OSTI ID:
5645019
Journal Information:
Journal of the Atmospheric Sciences; (United States), Journal Name: Journal of the Atmospheric Sciences; (United States) Vol. 50:21; ISSN 0022-4928; ISSN JAHSAK
Country of Publication:
United States
Language:
English