The abundance of H2 in Titan's troposphere from the Cassini CIRS investigation
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference45 articles.
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2. Titan's aerosol and stratospheric ice opacities between 18 and 500μm: vertical and spectral characteristics from Cassini CIRS;Anderson;Icarus,2011
3. The role of submicrometer aerosols and macromolecules in H2 formation in the Titan haze;Bakes;Icarus,2003
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1. Paleoclimate Evolution on Titan After Episodic Massive Methane Outgassing Simulated by a Global Climate Model;Journal of Geophysical Research: Planets;2021-12
2. On the H2 abundance and ortho-to-para ratio in Titan's troposphere;Icarus;2020-07
3. Hydrogen sensing in Titan's atmosphere: Motivations and techniques;Planetary and Space Science;2019-09
4. Cassini Composite Infrared Spectrometer (CIRS) Observations of Titan 2004–2017;The Astrophysical Journal Supplement Series;2019-09-01
5. Plate Section (PDF Only);Spectroscopy and Photochemistry of Planetary Atmospheres and Ionospheres;2019-02-14
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