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Fig. 20

image

Observed properties of the lower chromosphere from Model 1. Panel a: the averaged brightness temperature at K1 against the gas temperature at the temperature minimum is shown. The red solid line is y = x and the dashed line is the 3rd-degree polynomial fit. Panel b: the K2 peak separation against the column mass above the temperature rise is shown. The panels follow the same format as Fig. 6.

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