Search arXiv⌕ Search

arXiv · nlin/0303011

Initialization and the quasi-geostrophic slow manifold

Abstract

Atmospheric dynamics span a range of time-scales. The projection of measured data to a slow manifold, ${\cal M}$, removes fast gravity waves from the initial state for numerical simulations of the atmosphere. We explore further the slow manifold for a simple atmospheric model introduced by Lorenz and anticipate that our results will relevant to the vastly more detailed dynamics of atmospheres and oceans. Within the dynamics of the Lorenz model, we make clear the relation between a slow manifold $\cal M$ and the ``slowest invariant manifold'' ({\SIM}), which was constructed by Lorenz in order to avoid the divergence of approximation schemes for $\cal M$. These manifolds are shown to be identical to within exponentially small terms, and so the {\SIM} in fact shares the asymptotic nature of $\cal M$. We also investigate the issue of balancing initial data in order to remove gravity waves. This is a question of how to compute an ``initialized'' point on $\cal M$ whose subsequent evolution matches that from the measured initial data that in general lie off $\cal M$. We propose a choice based on the intuitive idea that the initialization procedure should not significantly alter the forecast. Numerical results demonstrate the utility of our initialization scheme. The normal form for Lorenz' atmospheric model shows clearly how to separate the dynamics of the different atmospheric waves. However, its construction demonstrates that {\em any} initialization procedure must eventually alter the forecast--the time-scale of the divergence between the initialized and the uninitialized solutions is inevitable and is inversely proportional to the square of initial level of gravity-wave activity.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

S. M. Cox, A. J. Roberts. 2003-03-07. Initialization and the quasi-geostrophic slow manifold. https://arxiv.org/abs/nlin/0303011

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

Intermittency-induced regimes in fast-slow dynamical systems

Intermittency is ubiquitous in nature and often arises from interactions between processes evolving on different time scales. We investigate whether, and how, intermittency in a fast system can be transmitted to a slower system that, in isolation, would settle onto a periodic regime. We address this in a unidirectionally coupled (skew-product) setting using two models of increasing complexity: coupled Lorenz-63 systems and coupled Kuramoto-Sivashinsky equations, in which the fast driving subsystem exhibits type-I intermittency. Increasing the driver's burst frequency progressively displaces the response attractor from its unforced limit cycle, until saturation. The induced regimes are jointly controlled by the coupling strength $C$ and the time-scale separation $τ$, which we explore through the variance of ensemble maxima, power spectra, extreme value statistics and phase-locking indices. In the Lorenz-63 model, $C$ mainly governs the loss of periodicity and the statistics of extremes, while $τ$ mainly governs the reshaping of the response spectrum; in the Kuramoto-Sivashinsky model these roles are less separable. In both systems, the transition to the intermittency-dominated regime is marked by heavy-tailed (Fréchet-type) extremes, which give way to bounded statistics at stronger coupling. The response delay, estimated via time-lagged mutual information, decreases exponentially as the two time scales become comparable. We identify phase synchronization during the driver's laminar phases as the mechanism behind several regime transitions, with chaotic bursts repeatedly breaking an otherwise stable locking. These results shed light on how fast intermittent variability, such as atmospheric forcing, may shape slower climate components such as the ocean or sea ice.

nlin.CD↗

Trajectory arclength reveals chaos

In this paper, we investigate the time-averaged phase space arclength of a trajectory, expressed through a normalized Lagrangian descriptor, as a trajectory-based diagnostic for distinguishing regular and chaotic dynamics. The proposed indicator, $Ω$, is computed by integrating the equations of motion together with a single scalar arclength-accumulation equation and therefore does not require variational equations, neighboring trajectories, or spatial derivatives of a Lagrangian descriptor field. Using Birkhoff's ergodic theorem together with estimates for quasiperiodic motion and correlation-based arguments for chaotic ergodic dynamics, we show that regular and chaotic trajectories exhibit different finite-time behavior despite the convergence of $Ω$ in both regimes. For quasiperiodic trajectories with Diophantine frequency vectors, deviations from the limiting average decay as $\mathcal{O}(τ^{-1})$, whereas sufficiently mixing chaotic dynamics exhibit root-mean-square fluctuations of order $τ^{-1/2}$ under suitable correlation assumptions. This difference in finite-time convergence and fluctuation scaling provides the theoretical basis for using $Ω$ to discriminate between the two dynamical regimes. We validate the proposed approach in the Hénon--Heiles and Fermi--Pasta--Ulam systems, comparing the resulting classification of initial conditions with SALI as a reference chaos indicator. The results support $Ω$ as a complementary single-trajectory diagnostic for chaos detection and as a practical source of scalar features for the analysis of trajectory ensembles, particularly in settings involving large numbers of trajectories or high-dimensional systems.

nlin.CD↗

Relativistic Quantum Chaos in Neutrino Billiards

Neutrino billiards serve as a model system for the study of aspects of relativistic quantum chaos. These are relativistic quantum billiards consisting of a spin-1/2 particle which is confined to a planar domain by imposing boundary conditions on the spinor components which were proposed in [Berry and Mondragon, {\it Proc. R. Soc.} A {\bf 412}, 53 (1987)]. We review their general features and the properties of neutrino billiards with shapes of billiards with integrable dynamics. Furthermore, we review the features of two neutrino billiards with the shapes of billiards generating a chaotic dynamics, whose nonrelativistic counterpart exhibits particular properties. Finally we briefly discuss possible experimental realizations of relativistic quantum billiards based on graphene billiards, that is, finite-size sheets of graphene.

nlin.CD↗