THE VARIABILITY OF HCN IN TITAN’S UPPER ATMOSPHERE AS IMPLIED BY THE CASSINI ION-NEUTRAL MASS SPECTROMETER MEASUREMENTS
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/2041-8205/826/1/L5/pdf
Reference39 articles.
1. Distribution of HCN in Titan’s upper atmosphere from Cassini/VIMS observations at 3μm
2. Mapping Magnetospheric Equatorial Regions at Saturn from Cassini Prime Mission Observations
3. Simulating the one-dimensional structure of Titan's upper atmosphere: 1. Formulation of the Titan Global Ionosphere-Thermosphere Model and benchmark simulations
4. Titan's Atmosphere from Voyager Infrared Observations
5. Titan’s atmosphere from ISO mid-infrared spectroscopy
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1. The Composition and Chemistry of Titan’s Atmosphere;ACS Earth and Space Chemistry;2024-02-29
2. Laboratory generation of hazes in Titan's upper atmosphere using ECR plasma;Planetary and Space Science;2023-05
3. Variability in Titan’s Mesospheric HCN and Temperature Structure as Observed by ALMA;The Planetary Science Journal;2022-06-01
4. Temperature Variability in Titan's Upper Atmosphere: The Role of Wave Dissipation;Journal of Geophysical Research: Planets;2020-06
5. Dayside nitrogen and carbon escape on Titan: the role of exothermic chemistry;Astronomy & Astrophysics;2019-12-20
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