Seasonal changes in the vertical structure of ozone in the Martian lower atmosphere and its relationship to water vapor

The mid-infrared channel of the Atmospheric Chemistry Suite (ACS MIR) onboard the ExoMars Trace Gas Orbiter is capable of observing the infrared absorption of ozone (O3) in the atmosphere of Mars. During solar occulations, the 003←000 band (3,000-3,060 cm−1) is observed with spectral sampling of ∼0....

Полное описание

Библиографические подробности
Главные авторы: Olsen, KS, Fedorova, AA, Trokhimovskiy, A, Montmessin, F, Lefèvre, F, Korablev, O, Baggio, L, Forget, F, Millour, E, Bierjon, A, Alday, J, Wilson, CF, Irwin, PGJ, Belyaev, DA, Patrakeev, A, Shakun, A
Формат: Journal article
Язык:English
Опубликовано: Wiley 2022