A Multiscale Model for the Modulation and Rectification of the ITCZ

Abstract

Abstract The authors introduce the modulation of the ITCZ equations (M-ITCZ), which describes the multiscale dynamics of the ITCZ on diurnal to monthly time scales in which mesoscale convectively coupled Rossby waves in the ITCZ are modulated by a large-scale gravity wave that is also generated by convection. Westward-propagating disturbances are observed to cause ITCZ breakup over the course of a few days, and the M-ITCZ meso-/planetary-scale coupled waves provide a mechanism for this interaction, thereby providing a framework to study the modulation and rectification of the Hadley circulation over long zonal length scales in the ITCZ. The authors consider examples of zonally symmetric heating profiles in the M-ITCZ system and generate a Hadley circulation consistent with the observed winds. Zonally localized heating creates a wind response throughout the tropics that is carried by a pair of zonally propagating gravity bores driving mean easterlies at the base and mean westerlies at the top of the troposphere. The bores carry low-temperature and upward velocity perturbations to the west of the heating and high-temperature and downward velocity perturbations to the east, making the westward-propagating branch favorable to convective triggering and the eastward-propagating branch favorable to convective suppression. The mesoscale dynamics of the M-ITCZ describe convectively forced, nonlinear Rossby waves propagating in the zonal winds created by the planetary-scale gravity wave. The authors suggest that convective coupling slows the westward-propagating gravity wave, thereby creating a coupled gravity–Rossby wave that is similar to the westward-propagating disturbances seen in the ITCZ.