Fig. 12
From: Characterising the three-dimensional ozone distribution of a tidally locked Earth-like planet
Comparative view of four different phases of the \({\mathrm{TOC}}_\mathrm{{PDE}}\) and \({\mathrm{TOC}}_\mathrm{{TLE}}\). a \(\varphi = 0\)° of \({\mathrm{TOC}}_{\mathrm{PDE}}\), b \(\varphi = 90\)° of \({\mathrm{TOC}}_{\mathrm{PDE}}\), c \(\varphi = 180\)° of \({\mathrm{TOC}}_{\mathrm{PDE}}\), d \(\varphi = 270\)° of \({\mathrm{TOC}}_{\mathrm{PDE}}\), e \(\varphi = 0\)° of \({\mathrm{TOC}}_{{\mathrm{TLE}}}\), f \(\varphi = 90\)° of \({\mathrm{TOC}}_{\mathrm{TLE}}\), g \(\varphi = 180\)° of \({\mathrm{TOC}}_{\mathrm{TLE}}\) and h \(\varphi = 270\)° of \({\mathrm{TOC}}_{{\mathrm{TLE}}}\). The antisolar point is indicated with a white point. The subsolar point is indicated with a black point