Dynamical propagation and growth mechanisms for convectively coupled equatorial Kelvin waves over the Indian Ocean

Convectively coupled equatorial Kelvin waves (CCKWs) are high‐impact tropical weather systems that can lead to severe flooding over the Maritime Continent. Here, a vorticity budget for CCKWs over the Indian Ocean is constructed using reanalysis data, to identify the basic mechanisms of eastward prop...

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Veröffentlicht in:Quarterly journal of the Royal Meteorological Society 2021-10, Vol.147 (741), p.4310-4336
1. Verfasser: Matthews, Adrian J.
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Sprache:eng
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Zusammenfassung:Convectively coupled equatorial Kelvin waves (CCKWs) are high‐impact tropical weather systems that can lead to severe flooding over the Maritime Continent. Here, a vorticity budget for CCKWs over the Indian Ocean is constructed using reanalysis data, to identify the basic mechanisms of eastward propagation and growth. The budget is reasonably well closed, with a small residual/subgrid‐scale term. In the lower troposphere, CCKWs behave like strongly modified theoretical equatorial Kelvin waves. Vortex stretching, from the divergence of the Kelvin wave acting on planetary vorticity (the −fD term), is the sole mechanism by which the vorticity structure of a theoretical Kelvin wave propagates eastward. In the lower and middle troposphere, this term is also the key mechanism for the eastward propagation of CCKWs but, due to subtleties in its structure and phasing linked to a combination of modal structures, it also contributes to growth. Unlike in the theoretical Kelvin wave, other vorticity source terms also play a role in the propagation and growth of CCKWs. In particular, vortex stretching from relative vorticity (the −ζD term) is the largest source term, and this leads strongly to growth, through interactions between the background and perturbation vorticity and divergence. Horizontal vorticity advection by the background flow contributes to propagation, and also acts to retard the growth of the CCKW. The sum of the source terms in this complex vorticity budget leads to eastward propagation and growth of CCKWs. The structure and vorticity budget of CCKWs in the upper troposphere is quite unlike that of a Kelvin wave, and appears to arise as a forced response to the lower‐tropospheric structure. The implications for numerical weather prediction and climate simulations are discussed. Convectively coupled Kelvin waves (CCKWs) are an important tropical weather system. Their underlying dynamics are often assumed to be the same as theoretical equatorial Kelvin waves. The vorticity budget of CCKWs presented here shows that the main mechanism for eastward propagation is vortex stretching of planetary vorticity, as in the theoretical wave, but zonal advection of basic state relative vorticity is also important. The main growth mechanism for CCKWs is vortex stretching of relative vorticity, with an interaction between the background state and the CCKW perturbation.
ISSN:0035-9009
1477-870X
DOI:10.1002/qj.4179