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Clouds and Hazes in Planetary Atmospheres

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Figure

Table 2.1: Model Parameters
Figure 2.1: Model temperature (rectangles) and pressure (short lines) profiles takenfrom the Venus International Reference Atmosphere (Seiff, Schofield, et al., 1985).
Figure 2.2: Model production rate profiles for sulfuric acid vapor (short lines)and photochemical condensation nuclei (rectangles), based on that of Imamura andHashimoto (2001) with the peak rates adjusted to fit LCPS data.
Figure 2.3: Model water vapor profile (rectangles) plotted with the Model A (filledcircles) and Venera 11, 13, and 14 data (triangles) from Ignatiev et al
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