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Photochemistry on Pluto: part II HCN and nitrogen isotope fractionation

We have converted our Titan one-dimensional photochemical model to simulate the photo- chemistry of Pluto’s atmosphere and include condensation and aerosol trapping in the model. We find that condensation and aerosol trapping are important processes in producing the HCN altitude profile observed by...

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Dades bibliogràfiques
Publicat a:Mon Not R Astron Soc
Autors principals: Mandt, Kathleen, Luspay-Kuti, Adrienn, Hamel, Mark, Jessup, Kandis-Lea, Hue, Vincent, Kammer, Josh, Filwett, Rachael
Format: Artigo
Idioma:Inglês
Publicat: 2017
Matèries:
Accés en línia:https://ncbi.nlm.nih.gov/pmc/articles/PMC6525008/
https://ncbi.nlm.nih.gov/pubmed/31105342
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1093/mnras/stx1587
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