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An attempt to detect transient changes in Io's SO 2 and NaCl atmosphere

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Academic year: 2021

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Fig. 2. Disk-averaged spectra (red) of the four SO 2 lines (left four columns) and the NaCl 260.223 GHz line (rightmost column) for the four IRAM observing tracks
Fig. 3. Comparison of various measurements obtained in the period from 15 Nov 2016 until 15 May 2017 that are possibly related to Io’s atmosphere: (a) Gemini images (3.8 μm) of volcanic hot spots on the hemisphere (CML in white) observed by IRAM (Table 1)

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