Decomposition of the model, for each count-rate state, into the radiation of the corona, which can be directly observed (dotted); the radiation reflected by the disc reaching the observer (dashed); the sum of both (dashed-dotted); and this sum partially absorbed (solid). Upper, middle, and bottom panels: low, medium and high count-rate states, respectively. As the covering fraction in the high regime is zero, there is no absorption of the emitted primary and reflected spectra. The Galactic foreground absorption is not shown in this plot.