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Vertical Temperature Structure in Io’s Atmosphere from ALMA SO2 Observations

  • Authors: Timothy N. Proudkii, Katherine de Kleer, Imke de Pater, Alexander E. Thelen, Statia Luszcz-Cook, Emmanuel Lellouch, Arielle Moullet

Timothy N. Proudkii et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 2.

Model comparison for the SO2 transition at 430.194 GHz from M22-L. The observed spectrum (black points with error bars) is overlaid with best-fit model spectra for the three tested TPs: 3T (left), 2T (middle), and 1T (right). The red bar in the upper right corner of the right column indicates the ALMA spectral resolution (FWHM). Residuals are shown in the bottom row.

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