资源环境科技发展态势分析平台

An equatorial heat source mimicking the strong diabatic heating above the west Pacific is added to an idealized, dry general circulationmodel. For small (<0.5Kday(-1)) heating rates the responses closelymatch the expectations fromlinear Matsuno-Gill theory, though the amplitudes of the responses increase sublinearly. This "linear'' regime breaks down for larger heating rates and it is found that this is because the stability of the tropical atmosphere increases. At the same time, the equatorial winds increasingly superrotate. This superrotation is driven by stationary eddy momentum fluxes by the waves excited by the heating and is damped by the vertical advection of lowmomentum air by the mean flow and, at large heating rates, by the divergence of momentum by transient eddies.

These dynamics are explored in additional experiments in which the equator-to-pole temperature gradient is varied. Very strong superrotation is produced when a large heating rate is applied to a setup with a relatively weak equator-to-pole temperature gradient, though there is no evidence that this is a case of "runaway'' superrotation.