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Computation of Atmospheric Concentrations of Molecular Clusters from ab initio Thermochemistry
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Monóxido de carbono en Júpiter y sus implicaciones para la convección atmosférica

R G Prinn, S S Barshay

    Science (New York, N.Y.)
    |December 9, 1977
    PubMed
    Resumen

    El monóxido de carbono en la atmósfera de Júpiter se mezcla rápidamente desde capas profundas y calientes. Esto indica una convección muy rápida impulsada por el calor interno, que apoya las teorías dinámicas planetarias.

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