Fig. 9.
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Hydrostatic and thermal equilibrium along the field line with gravity for Hildner’s function. The background heating is E0 = 5 × 10−7 W m−3 and hch = 35, 15, 0 for the continuous, dashed, and dotted lines. In this particular example T0 = 104 K, ρ0 = 10−11 kg m−3 and the temperature threshold for the imposed chromosphere is 104 K. Model A is used in this example.
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