Docstoc

Dynamics of Resonantly Interacting Equatorial Waves

Document Sample
Dynamics of Resonantly Interacting Equatorial Waves Powered By Docstoc
					                 Dynamics of Resonantly Interacting Equatorial Waves



                                 Carlos Frederico M. Raupp
                            Department of Atmospheric Sciences
               Institute of Astronomy, Geophysics and Atmospheric Sciences
                      University of São Paulo - São Paulo/SP – Brazil
                           e-mail: cfmraupp@model.iag.usp.br

                                           Abstract

This work explores some dynamical features on the nonlinear interactions among equatorial
waves. The shallow-water equation model with the equatorial -plane approximation is
used for this purpose. The Galerkin method is applied to the governing equations with the
basis functions given by the eigensolutions of the linear problem. From the phase space
expansion of two particular integrals of motion of the system, quadratic to lowest order,
some constraints are obtained for which the coupling coefficients must satisfy in order to
ensure the invariance of such integrals. From the numerical evaluation of the coupling
coefficients, these constraints are used to determine the possible resonant triads among
equatorial waves. Numerical integrations of the resonant 3-wave problem show that the
energy of the waves in a resonant triad evolves periodically in time, with the period and
amplitude of the energy oscillations dependent on magnitude of the initial amplitudes of the
waves and the way in which the initial energy is distributed among the triad components.
The high frequency modes are found to be energetically more active than the low frequency
ones. The latter tend to act as “catalyst” components in a resonant triad. Integrations of the
problem of 2 resonant triads coupled by one mode point out the importance of gravity
waves in the inter-triad energy exchange, suggesting the significance of these modes in the
redistribution of energy throughout the atmospheric motion spectrum. The results also
show that the inter-triad energy exchange provided by the highest frequency mode of two
triads occurs in a longer time scale than the intra-triad interactions. Therefore, these results
also suggest the importance of the high frequency modes in the generation of the low
frequency variability (intra-seasonal or even longer period variability) of the atmospheric
flow.

				
DOCUMENT INFO
Shared By:
Categories:
Tags:
Stats:
views:3
posted:1/2/2011
language:English
pages:1