Context images for Venus Express radio occultation measurements: A search for a correlation between temperature structure and UV contrasts in the clouds of Venus

Open Access

Fig. 11

RFR versus temperature (left) and normalised temperature (right) at 67 km altitude. Normalisation was done relative to a linear least square fit to the temperature as a function of latitude at each level between 50 and 80 km altitude. See Figs. 8 and 9.

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