Volume emission rate profiles at a solar zenith angle of 0^◦ for Raman-scattered Lyα photons, i.e. photons scattered from Lyα to 1280 Å by H₂. These photons can be scattered again by H₂ (Rayleigh scattering at 1280 Å) and contribute to the 1280 Å brightness of Uranus. The solid lines in the left and right panels show the absolute and cumulative volume emission rates, respectively, for the Raman-scattered Lyα photons in atmospheres with the three best-fit methane profiles that reproduce the observed Raman feature brightness of ${20}_{-6}^{+1}$ R. The dashed lines indicate the altitude at which ${\tau }_{\text{abs}}^{1216}=1$ for atmospheres with corresponding methane profile.