Abstract
The spiral bands that occur in tropical cyclones can be conveniently divided into two classes - outer bands and inner bands. Evidence is presented here that the outer bands form as the result of nonlinear effects during the breakdown of the intertropical convergence zone (ITCZ) through barotropic instability. It is argued that inner bands form in a different manner. As a tropical cyclone intensifies due to latent heat release, the PV field becomes nearly circular with the highest values of PV in the cyclone center. The radial gradient of PV provides a state on which PV waves (the generalization of Rossby waves) can propagate. The nonlinear breaking of PV waves then leads to an irreversible distortion of the PV contours and a downgradient flux of PV. The resulting vortex is generally larger in horizontal extent and exhibits a spiral band of PV. When the formation of outer and inner bands is interpreted in the context of a normal-mode spectral model, they emerge as slow manifold phenomena; that is, they have both rotational and (balanced or slaved) gravitational mode aspects. -from Authors
Cite
CITATION STYLE
Guinn, T. A., & Schubert, W. H. (1993). Hurricane spiral bands. Journal of the Atmospheric Sciences, 50(20), 3380–3403. https://doi.org/10.1175/1520-0469(1993)050<3380:HSB>2.0.CO;2
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