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- W2030632917 abstract "The intensity of Jupiter's He 584 Å airglow has been measured by the Voyager U.V. spectrometers. The disc-averaged brightness is about 4 Rs and limb darkening is present. The intensity probably varies with longitude, the variation being out of phase with the H Lyman-α intensity bulge. Modelling of resonance scattering of the solar He 584 Å line by Jupiter's atmosphere has shown that the hydrogen and helium emissions can be explained about equally well by at least two self-consistent scenarios involving the structure (temperature and eddy diffusion coefficient) and excitation of the atmosphere. All our evidence points to a dramatic change of conditions in the Jovian atmosphere in the time between Pioneer and Voyager encounters." @default.
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- W2030632917 date "1981-03-01" @default.
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- W2030632917 title "Voyager U.V. spectrometer observations of He 584 Å dayglow at Jupiter" @default.
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- W2030632917 doi "https://doi.org/10.1016/0032-0633(81)90015-5" @default.
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