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Microwave Remote Sensing of Giant Planet Atmospheres: Considerations for Saturn and Uranus Orbiter Missions

  • Authors: Alex B. Akins, Mark D. Hofstadter

Alex B. Akins and Mark D. Hofstadter 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

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.

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