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astro-ph.SR2025
Heat Transport and Dissipation in 2.5D Rotating Internally Heated and Cooled Convection
Tom Joshi-Hartley, Matthew K. Browning, Laura K. Currie +3
Models of astrophysical convection, such as mixing length theory, typically assume that the heat transport is independent of microphysical diffusivities. Such 'diffusion-free' beha…
astro-ph.SR2009★ 88 cited
Exploring the vs relation with flux transport dynamo models of solar-like stars
L. Jouve, B. P. Brown, A. S. Brun
Aims: To understand stellar magnetism and to test the validity of the Babcock-Leighton flux transport mean field dynamo models with stellar activity observations Methods: 2-D mean…