Fig. 10
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Distributions of CH4, NH3, C2H2, and HCN during and ~1 month after a flare event of total energy 2 × 1032 erg (upper row), 2 × 1033 erg (middle row) and 2 × 1034 erg (lower row). From left to right: substellar point, evening limb, antistellar point and morning limb. The pre-flare distributions are represented by the black dotted lines.
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