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Earth, Planets and Space
Fig. 21 | Earth, Planets and Space

Fig. 21

From: Effects of variation in coagulation and photochemistry parameters on the particle size distributions in the Venus clouds

Fig. 21

Left: The total column abundance in the microphysical model domain (40–80 km) for each latitude and coagulation condition simulated here. Right: Mass loading and effective radius at 46.5 km and ‘pol2’ profile in the temperature-dependent coagulation simulation, focusing on the time from 950 to 1050 days, showing the nature of the evolution seen in the simulation

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