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physics.flu-dyn2026
Internal heating in rapidly rotating convection is not a shortcut to geostrophic turbulence
Justin A. Nicoski, Tobias G. Oliver, Stefano Maffei +1
Convective turbulence in planets and stars is often driven by internal heating. This forcing mechanism has also been proposed as a means of accessing the diffusion-free scalings of…
physics.flu-dyn2026
Rapidly rotating internally heated convection: bounds on long-time averages
Yutong Zhang, Ali Arslan, Stefano Maffei +1
Convection on geophysical and astrophysical scales is subject to rapid rotation and strong heating from within the domain. In studying the long-time behaviour of the solutions for…