Open Access
Table 2
Models discussed in this work.
| Model | Description |
|---|---|
| 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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