Spatial variations in Titan’s atmospheric temperature: ALMA and Cassini comparisons from 2012 to 2015
Submillimeter emission lines of carbon monoxide (CO) in Titan's atmosphere provide excellent probes of atmospheric temperature due to the molecule's long chemical lifetime and stable, well constrained volume mixing ratio. Here we present the analysis of 4 datasets obtained with the Atacama...
| Egile Nagusiak: | , , , , , , , , , |
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| Formatua: | Journal article |
| Argitaratua: |
Elsevier
2017
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