Abundance measurements of Titan’s stratospheric HCN, HC3N, C3H4, and CH3CN from ALMA observations
Previous investigations have employed more than 100 close observations of Titan by the Cassini orbiter to elucidate connections between the production and distribution of Titan’s vast, organic-rich chemical inventory and its atmospheric dynamics. However, as Titan transitions into northern summer, t...
| المؤلفون الرئيسيون: | , , , , , , , , |
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| التنسيق: | Journal article |
| منشور في: |
Elsevier
2018
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