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Fig. 4
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Evolution of CH4, NH3, C2H2, and HCN (top to bottom) on the substellar point, evening limb, antistellar point and morning limb (left to right) during the first ~2.3 days (Pwind/2) after the flare event that started on t = 0. The pre-flare distributions are represented by the black dashed-dotted lines.
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