Table 1
Identification classes, solar features, and atmosphere models utilized in this study.
| Class | Solar feature | Atmosphere model |
|
|
||
| B | quiet Sun | model B, VAL3-C, FAL3-C, FA-06 |
| D | network | model D, FAL3-F |
| F | enhanced | model F |
| network | ||
| H | plage | model H, model F, FAL3-F, FAL3-P |
| P | bright plage | model P |
| S | umbra | – |
| R | penumbra | – |
Notes. The table summarizes the classes utilized for the identification of the various solar features, the relation between each class and the corresponding solar feature, as well as the relation between solar features and atmosphere models considered for the comparisons presented in the following. Models B to P indicate the set of atmospheres of Fontenla et al. (2009), which constitutes the reference set in this study. Models VAL3-C, FAL3-C, and FA06-C indicate the atmospheres for quiet Sun regions presented by Vernazza et al. (1981), and Fontenla et al. (1993, 2006), respectively. Models FAL3-F and FAL3-P are the atmospheres for plage and bright plage regions presented by Fontenla et al. (1993).
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