Density, ρ (top), gas pressure, p_gas (middle), and temperature, T (bottom), for all magnetic field strengths and stellar types. The horizontal axis is the number of pressure scale heights below the surface computed for the SSD case for each star (the left side of the plot is toward the bottom boundary and the right side is toward the top). The vertical dotted line marks the height at which ⟨τ⟩ = 1 in each case.