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. Author manuscript; available in PMC: 2019 Mar 4.
Published in final edited form as: Icarus. 2015 Aug 14;261:149–168. doi: 10.1016/j.icarus.2015.08.012

Figure 9:

Figure 9:

The sensitivity of the C2H4 profile to the rate coefficient for reaction R134 (H + C2H4 + M →C2H5 + M) for pre-storm conditions (dotted lines) and the hot beacon core on May 4, 2011 (solid lines), for our nominal model (red) and a model in which the rate coefficient for R134 is taken from the recommendation of Li et al. (2014) (blue). The black square is our CIRS-derived C2H4 beacon-core abundance from May 4, 2011.