\[s\]). Silicates dominate the cloud particle volume by far with values of 45%$\,\ldots\,60\%$. High temperature condensates (\[s\], Fe\[s\], \[s\]) dominate the cloud particle volume at higher temperatures where silicates have evaporated. Carbon contributes a little bit, and salts (here KCl\[s\]) play no significant role for the material composition in the temperature ranges of the WASP-43b atmosphere investigated here. KCl did occur as a minor nucleation species in the northern hemisphere of the nightside of WASP-43b. A detailed account of the individual contributions of the 16 materials considered in our study is given in Fig. \[fig:matvolfrac\_ASP\] for the two terminators, the substellar and the anti-stellar point. We note that the terminator structures are rather comparable in the frame of the models applied here.

![Column integrated cloud properties for WASP-43b for 18 selected 1D profiles. [**Top:**]{} Nucleation rate shown $\int_{\rm zmin}^{\rm zmax} J_*(z) dz$ \[cm$^{-2}$ s$^{-1}$\] with $J_*=\sum_{\rm s} J_{\rm s}$ ($s=\,$, SiO, C, KCl) [**Middle:**]{} $\langle\langle a \rangle\rangle = (\int_{\rm zmin}^{\rm zmax} n_{\rm d}(z)\langle a(z) \rangle \,dz)/( \int_{\rm zmin}^{\rm zmax} n_{\rm d}(z) \,dz)$ \[$\mu$m\] with $n_{\rm d}(z)$ \[cm$^{-3}$\] the local cloud particle number density. [**Bottom:**]{} Material volume fraction: $\int_{\rm zmin}^{\rm zmax} (V_{\rm s}(z)/V_{\rm tot}(z))\,dz$. []{data-label="fig:<<a>>_Parm"}](images/column_Jstar_more_Parm.pdf "fig:"){width="50.00000%"} ![Column integrated cloud properties for 