Fig. A.1

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Comparison of the natural logarithm of the supersaturation level S from the representative mineral model (upper row) to the natural logarithm of the supersaturation level S given by GGCHEM for the different mineral species (lower row) in a gas with solar composition as a function of the temperature for two different pressure levels. The crosses in the upper row show the sublimation temperatures for P = 0.1 Pa while the circles show the sublimation temperatures for P = 104 Pa, In the lower row, the vertical dotted lines indicate the sublimation temperatures from the representative mineral model.
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