The ensemble-mean response of the annual mean ITCZ to CO2-induced warming is to shift to the north, amplifying the pre-existing asymmetry in the basic state, but the spread across models is large. This is consistent with a similarly large scatter in the warming differential between the hemispheres; the magnitude of the shift is also modulated by the input of energy into the equatorial atmosphere, which varies greatly across models. Overall, the inter-model variance in the annual mean changes in the position of the ITCZ is explained equally well by changes in the latitude of the energy flux equator and in the magnitude of the atmospheric energy flux across the equator. The models do not show that the relationship between seasonal excursion of the ITCZ and seasonal changes in energy transport is quantitatively the same as that found between annual mean changes in forced simulation; nevertheless, there is qualitative agreement between the behavior of all TRACMIP simulations and more realistic CMIP-like configurations.
The CO2-induced northward shift of the ITCZ is not uniform across the year, but is strongest during spring (when the climatological ITCZ is furthest to the south in these setups). The width of the ITCZ (defined as the region of net precipitation) is decreased in the annual mean, because of the sharp reduction in Southern Hemisphere precipitation during spring, but it actually increases during most months of the climatology.
We further explore how well the energetic frameworks proposed in the literature work in explaining forced changes in the seasonal cycle of the ITCZ and we diagnose what role changes in gross moist stability play in changing the seasonal relationship between energy transport and ITCZ position as the climate warms.