Are Martian clouds fractals?

Statistics – Methodology

Scientific paper

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Clouds (Meteorology), Fractals, Mars Atmosphere, Atmospheric Circulation, Atmospheric Composition, Earth Atmosphere, Image Analysis, Satellite Imagery, Viking Mars Program, Mars, Clouds, Images, Viking Missions, Theoretical Studies, Structure, Shape, Characteristics, Size, Atmosphere, Comparisons, Analysis, Composition, Hypotheses, Features, Procedure

Scientific paper

The hypothesis of Lovejoy (1982) on the fractal nature of terrestrial clouds and rain areas is applied to the Martian atmosphere. The validity of the hypothesis in the case of the Martian atmosphere is examined by analyzing selected photographic images obtained by the K Viking lander. The images show a number of cloud features on Mars including lee wave clouds, a bright 'cirrus' cloud, and several plume-like formations near the Arisia Mons. The methodology used to retrieve the area-perimeter correlations of the Martian clouds is described in detail. It is shown that the area-perimeter correlations of the Martian clouds are in good agreement with the predictions of Lovejoy, lending support to the theory that all clouds are fractals.

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