C3HX Hydrocarbon Abundance in Titan's Atmosphere from Cassini Infrared Spectra
Abstract
These first measured profiles of propylene in Titan's atmosphere show that the abundance of the gas differs from photochemical model predictions.
- Publication:
-
49th Annual Lunar and Planetary Science Conference
- Pub Date:
- March 2018
- Bibcode:
- 2018LPI....49.2376L