Fig. 8

Evolution of the H2O abundance profile in the stratosphere of Jupiter for y0 = 1.1 × 10−7 above a pressure level p0 = 0.2 mbar (SL9 parameters) and Kzz Model B. These profiles are obtained from the photochemical model and a comparison with the observations. The red dotted abundance profile represents the initial profile of H2O at the time of the SL9 comet impacts in 1994. Each solid curve represents the abundance profile of H2O at dates corresponding to Odin observations. The black dashed profile represents the abundance of H2O that we predict for 2030.
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