The origin of enhanced [Formula: see text] production from photoionized CO 2 clusters

CO -rich planetary atmospheres are continuously exposed to ionising radiation driving major photochemical processes. In the Martian atmosphere, CO clusters are predicted to exist at high altitudes motivating a deeper understanding of their photochemistry. In this joint experimental-theoretical study...

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Veröffentlicht in:Communications chemistry 2022-02, Vol.5 (1), p.16
Hauptverfasser: Ganguly, Smita, Barreiro-Lage, Dario, Walsh, Noelle, Oostenrijk, Bart, Sorensen, Stacey L, Díaz-Tendero, Sergio, Gisselbrecht, Mathieu
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Sprache:eng
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