Image Details
Caption: Figure 4.
Nadir brightness temperature (A, C) and limb-darkening spectra (B, D, R(θ) = ∣TB(0) − TB(50∘)∣/TB(0)) for atmospheric models of Saturn and Uranus in Figure 1. The effects of some arbitrary perturbations to this model are also illustrated.
© 2026. The Author(s). Published by the American Astronomical Society.