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...
Κύριοι συγγραφείς: | Thelen, A, Nixon, C, Chanover, N, Molter, E, Cordiner, M, Achterberg, R, Serigano, J, Irwin, P, Teanby, N, Charnley, S |
---|---|
Μορφή: | Journal article |
Έκδοση: |
Elsevier
2017
|
Παρόμοια τεκμήρια
Παρόμοια τεκμήρια
-
Abundance measurements of Titan’s stratospheric HCN, HC3N, C3H4, and CH3CN from ALMA observations
ανά: Thelen, A, κ.ά.
Έκδοση: (2018) -
ALMA OBSERVATIONS OF HCN AND ITS ISOTOPOLOGUES ON TITAN
ανά: Molter, E, κ.ά.
Έκδοση: (2016) -
Detection of cyclopropenylidene on Titan with ALMA
ανά: Nixon, CA, κ.ά.
Έκδοση: (2020) -
Isotopic ratios of carbon and oxygen in Titan's co using ALMA
ανά: Serigano, J, κ.ά.
Έκδοση: (2016) -
Mapping vinyl cyanide and other nitriles in Titan’s atmosphere using ALMA
ανά: Lai, J, κ.ά.
Έκδοση: (2017)