Image Details
Caption: Figure 8.
Ratios of the observed flux to the model for Juno, assuming uniform thermal and dielectric properties, with respect to longitude (left) and rotational phase, φ (right). The rotational phase follows ALMA Partnership et al. (2015). The error bars reflect the uncertainty in the flux measurement, not including any systematic uncertainty in the thermal model.
© 2026. The Author(s). Published by the American Astronomical Society.