Clouds, haze, and CH, CHD, HCN, and CH in the atmosphere of Titan probed via 3 ?m spectroscopy
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by 40 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Investigation of Titan’s South Polar HCN Cloud during Southern Fall Using Microphysical Modeling;The Planetary Science Journal;2023-12-01
2. Hydrocarbon chemistry in the atmosphere of a Warmer Exo-Titan;Frontiers in Astronomy and Space Sciences;2022-09-19
3. Variability in Titan’s Mesospheric HCN and Temperature Structure as Observed by ALMA;The Planetary Science Journal;2022-06-01
4. Line-strengths, collisional coefficients and narrowing parameters in the ν3 band of methane: H2, He, N2, O2, Ar and CO2 collider effects;Journal of Quantitative Spectroscopy and Radiative Transfer;2021-09
5. Investigating the Condensation of Benzene (C6H6) in Titan’s South Polar Cloud System with a Combination of Laboratory, Observational, and Modeling Tools;The Planetary Science Journal;2021-07-01
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