Low radar emissivity signatures on Venus volcanoes and coronae: New insights on relative composition and age

Multiple studies reveal that most of Venus highlands exhibit anomalously high radar reflectivity and low radar emissivity relative to the lowlands. This phenomenon is thought to be the result of atmosphere-surface interactions in the highlands, due to lower temperatures. These reactions are a functi...

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Veröffentlicht in:Icarus (New York, N.Y. 1962) N.Y. 1962), 2020-06, Vol.343, p.113693, Article 113693
Hauptverfasser: Brossier, J.F., Gilmore, M.S., Toner, K.
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Sprache:eng
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