The UMIST database for astrochemistry

By Y. L. Teuff. 2000

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Three‐dimensional Martian ionosphere model: I. The photochemical ionosphere below 180 km (2013, methodology): “…recommended by the 2012 edition of the University of Manchester Institute of Science and Technology Database for Astrochemistry astrochemistry.net [McElroy et al., 2013], with the exceptions of reactions I1, I3, I17, I19, I20, I21, I22, I23, I26, and I27, where we use the same rate as in Fox and…”
A photochemical model of Titan's atmosphere and ionosphere (2009, background): “…+ 7 + C3H2 → C10H+9 + hν 10−10 1.11+5 837 413b C10H + 9 + e → C10H8 + H 10−6, 0.5 1.68+6 629 414b C9H + 11 + e → C9H8 + H2 + H 10−6, 0.5 3.49+7 554 415b C10H + 11 + e → C10H8 + H2 + H 10−6, 0.5 1.04+6 156 a Rate coefficients are from McEwan and Anicich (2007); recombination rate coefficients are…”