Variability in Titan’s mesospheric HCN and temperature structure as observed by ALMA

Variability in Titan’s mesospheric HCN and temperature structure as observed by ALMA

The temperature structure of Titan's upper atmosphere exhibits large variability resulting from numerous spatially and temporally irregular external energy sources, seasonal changes, and the influence of molecular species produced via photochemistry. In particular, Titan's relatively abund...

Полное описание

Библиографические подробности
Главные авторы:	Thelen, AE, Nixon, CA, Cosentino, RG, Cordiner, MA, Teanby, NA, Newman, CE, Irwin, PG, Charnley, SB
Формат:	Journal article
Язык:	English
Опубликовано:	IOP Publishing 2022

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