Fig. 7
Upper panel: production rates of neutral species NO, N(4S), H, OH and O due to ion-chemistry processes calculated with ExoTIC (black lines) for scenario 2 (GLE05) compared to theoretical values of existing parameterizations (coloured dots, see text). Lower panel: production rates of NO, N(4 S), H, OH and O due to ion-chemistry processes in the atmosphere for scenario 1 (quiescent Sun, black lines) and scenario 2 (GLE05, green lines).
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