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Table C.1.
Best fit models according to Mahalanobis distance.
| Grid | Observables | Pattern construction | Mini [M⊙] | Zini | αCBM | fCBM | log(Denv) | Xc |  |
MD | AICc(MD) |
|---|---|---|---|---|---|---|---|---|---|---|---|
| Radiative | ΔP | Longest sequence | 3.5 | 0.023 | 0.2 | 0.0 | 0.0 | 0.44 | 3479 | 182 | −294.0 |
| Highest amplitude | 3.5 | 0.023 | 0.2 | 0.0 | 0.0 | 0.44 | 3479 | 186 | −290.6 | ||
| Highest frequency | 3.5 | 0.023 | 0.2 | 0.0 | 0.0 | 0.44 | 3479 | 184 | −293.6 | ||
| Period | Longest sequence | 3.5 | 0.023 | 0.2 | 0.0 | 0.0 | 0.44 | 362 028 | 168 | −315.8 | |
| Highest amplitude | 3.5 | 0.023 | 0.2 | 0.0 | 0.0 | 0.44 | 362 028 | 173 | −313.4 | ||
| Highest frequency | 3.5 | 0.023 | 0.2 | 0.0 | 0.0 | 0.44 | 362 028 | 170 | −315.2 | ||
| Péclet | ΔP | Longest sequence | 3.4 | 0.023 | 0.05 | 0.0 | 0.5 | 0.40 | 2398 | 230 | −255.7 |
| Highest amplitude | 3.2 | 0.023 | 0.15 | 0.005 | 0.0 | 0.40 | 1616 | 246 | −241.1 | ||
| Highest frequency | 3.3 | 0.023 | 0.0 | 0.0 | 0.5 | 0.40 | 2450 | 241 | −247.3 | ||
| Period | Longest sequence | 3.4 | 0.023 | 0.05 | 0.0 | 0.5 | 0.40 | 744 142 | 218 | −276.5 | |
| Highest amplitude | 3.2 | 0.023 | 0.15 | 0.005 | 0.0 | 0.40 | 101 511 | 226 | −270.6 | ||
| Highest frequency | 3.2 | 0.023 | 0.15 | 0.005 | 0.0 | 0.40 | 101 511 | 233 | −263.9 | ||
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