Models discussed in this work.
|A||The base low-resolution model, in which the deep atmosphere is isothermally initialised|
|B||Like model A, but with the deep atmosphere adiabatically initialised|
|C||Mid-resolution version of model A (d = 30)|
|D||High-resolution version of model A (d = 40)|
|E →I||Highly evolved versions of model A, which have reached a deep adiabat and then had deep isothermal Newtonian cooling introduced at various strengths: For E log(τ220) = 7.5, F log(τ220) = 11, G log(τ220) = 15, H log(τ220) = 20, and I log(τ220) = 22.5|
|J & K||Highly evolved versions of model A which have reached a deep adiabat, and then had their outer atmospheric Newtonian cooling modified to reflect a different surface temperature: 1200 K in model J and 2200 K in model K|
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