Idealized nonrotating simulations show spontaneous zonal convective self-aggregation of an ITCZ-like rain belt occurs preferentially at high peak SST and large meridional SST amplitude, linked to weakened meridional inflow, enhanced lower-tropospheric stability, and large imposed meridional MSE-for
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Spontaneous Zonal Symmetry Breaking of Tropical Rain Belt
Idealized nonrotating simulations show spontaneous zonal convective self-aggregation of an ITCZ-like rain belt occurs preferentially at high peak SST and large meridional SST amplitude, linked to weakened meridional inflow, enhanced lower-tropospheric stability, and large imposed meridional MSE-for