A survey and investigation of 'stealth' coronae on Venus - Distribution, morphology, and stratigraphy

Mathematics – Logic

Scientific paper

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Venus Surface, Coronas, Planetary Structure, Stratigraphy, Photogeology, Geological Surveys, Morphology, Photomapping

Scientific paper

Initial Scarpellini Quadrangle survey results indicate that stealth coronae are usually circular in plan and between 160 and 1700 km in diameter. Many of them consist of a circular topographic ridge, approximately 30 to 50 km across and rising 200 to 700 m above the surrounding surface. Stealth coronae have also been found to have formed in a variety of geological units, including regional plains materials and lineated and mottled plains materials. It is inferred that the features are not confined to a single epoch of Venusian geological evolution.

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