Exploring the Lyapunov instability properties of high-dimensional atmospheric and climate models
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Published:2018-05-28
Issue:2
Volume:25
Page:387-412
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ISSN:1607-7946
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Container-title:Nonlinear Processes in Geophysics
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language:en
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Short-container-title:Nonlin. Processes Geophys.
Author:
De Cruz LesleyORCID, Schubert Sebastian, Demaeyer JonathanORCID, Lucarini ValerioORCID, Vannitsem StéphaneORCID
Abstract
Abstract. The stability properties of intermediate-order climate models are
investigated by computing their Lyapunov exponents (LEs). The two models
considered are PUMA (Portable University Model of the Atmosphere), a
primitive-equation simple general circulation model, and MAOOAM (Modular
Arbitrary-Order Ocean-Atmosphere Model), a quasi-geostrophic coupled
ocean–atmosphere model on a β-plane. We wish to investigate the
effect of the different levels of filtering on the instabilities and dynamics
of the atmospheric flows. Moreover, we assess the impact of the oceanic
coupling, the dissipation scheme, and the resolution on the spectra of LEs. The PUMA Lyapunov spectrum is computed for two different values of the
meridional temperature gradient defining the Newtonian forcing to the
temperature field. The increase in the gradient gives rise to a higher
baroclinicity and stronger instabilities, corresponding to a larger dimension
of the unstable manifold and a larger first LE. The Kaplan–Yorke dimension
of the attractor increases as well. The convergence rate of the rate function
for the large deviation law of the finite-time Lyapunov exponents (FTLEs) is
fast for all exponents, which can be interpreted as resulting from the
absence of a clear-cut atmospheric timescale separation in such a model. The MAOOAM spectra show that the dominant atmospheric instability is
correctly represented even at low resolutions. However, the dynamics of the
central manifold, which is mostly associated with the ocean dynamics, is not
fully resolved because of its associated long timescales, even at
intermediate orders. As expected, increasing the mechanical atmosphere–ocean
coupling coefficient or introducing a turbulent diffusion parametrisation
reduces the Kaplan–Yorke dimension and Kolmogorov–Sinai entropy. In all
considered configurations, we are not yet in the regime in which one can
robustly define large deviation laws describing the statistics of the FTLEs. This paper highlights the need to investigate the natural variability of the
atmosphere–ocean coupled dynamics by associating rate of growth and decay of
perturbations with the physical modes described using the formalism of the
covariant Lyapunov vectors and considering long integrations in order to
disentangle the dynamical processes occurring at all timescales.
Publisher
Copernicus GmbH
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