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Earth, Planets and Space
Fig. 9 | Earth, Planets and Space

Fig. 9

From: An uppermost haze layer above 100 km found over Venus by the SOIR instrument onboard Venus Express

Fig. 9

(A) Separation of the Sun region into different zones for one detector pixel as a function of the index, i.e., the time after the beginning of the measurement. Lines corresponding to specific tangent altitudes are plotted. (B) Plot of the fit over the S region and extrapolation in the T region. The graph inside shows the residuals of the fit (taken from Trompet et al. 2016)

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