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- W2025112091 abstract "Abstract A modified Eddington approximation is presented which describes radiative transfer due to the pressure-induced far infrared spectrum of hydrogen. When applied to the atmospheres of the major planets, the radiative transfer model produces atmospheric temperature profiles which are in good agreement with more detailed calculations. Solar absorption and infrared transmission by the fundamental bands of methane are further included for Jupiter and Saturn, resulting in a temperature inversion within both atmospheres above an altitude corresponding to a pressure of roughly 0.01 atm. This relatively high inversion region appears to be qualitatively consistent with infrared observations of methane and ammonia bands for Jupiter. Additional sources of solar absorption, consisting of the pressure-induced vibration-rotation bands of hydrogen and the overtones of the v3 methane fundamental, are shown to have a minor effect upon the atmospheric thermal structure for Jupiter and Saturn." @default.
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- W2025112091 title "Radiative transfer within the atmospheres of the major planets" @default.
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