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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 9.

Observed and modeled SO2 rotational line spectra for all datasets. Each row corresponds to a specific dataset and TP parameterization, as labeled (M22-L: 3T; J21-L: 3T; M22-T: 1T; and J21-T: 1T). Individual panels show the targeted SO2 transitions, which are labeled by their rest frequency ν0 and centered in frequency space. Observed spectra are plotted as black points. The best-fit model is overlaid as a dark-gray line, with the lighter shading indicating the 1σ uncertainty.

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