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• W2026842595 abstract "The abundances of PH3, CH3D, and GeH4 are derived from the 2100- to 2250-cm−1 region of the Voyager 1 IRIS spectra. No evidence is seen for large-scale variations of the phosphine abundance over Jovian latitudes between −30 and +30°. In the atmospheric regions corresponding to 170–200°K, the derived PH3/H2 value is (4.5 ± 1.5) × 10−7 or 0.75 ± 0.25 times the solar value. This result, compared with other PH3 determinations at 10 μm, suggests than the PH3/H2 ratio on Jupiter decreases with atmospheric pressure. In the 200–250°K region, we derive, within a factor of 2, CH3D/H2 and GeH4/H2 ratios of 2.0 × 10−7 and 1.0 × 10−9, respectively. Assuming a C/H value of 1.0 × 10−3, as derived from Voyager, our CH3D/H2 ratio implies a D/H ratio of 1.8 × 10−5, in reasonable agreement with the interstellar medium value." @default.
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• W2026842595 date "1982-03-01" @default.
• W2026842595 modified "2023-10-14" @default.
• W2026842595 title "An estimate of the PH3, CH3D, and GeH4 Abundances on Jupiter from the Voyager IRIS data at 4.5 μm" @default.
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• W2026842595 doi "https://doi.org/10.1016/0019-1035(82)90046-x" @default.
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