New constraints on Titan's stratospheric n-butane abundance

Curiously, n-butane has yet to be detected at Titan, though it is predicted to be present in a wide range of abundances that span over 2.5 orders of magnitude. We have searched infrared spectroscopic observations of Titan for signals from n-butane (n-C4H10) in Titan's stratosphere. Three sets o...

詳細記述

書誌詳細
主要な著者: Steffens, BL, Nixon, CA, Sung, K, Irwin, PGJ, Lombardo, NA, Pereira, E
フォーマット: Journal article
言語:English
出版事項: American Astronomical Society 2022

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