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- W2075492634 abstract "The Voyager 2 Ultraviolet Spectrometer (UVS) stellar and solar occultation data obtained at Uranus have been analyzed to infer smooth thermospheric temperature profiles and heat source characteristics. Temperatures inferred in the upper thermosphere from these occultations are much higher (850 ± 100 K) than can be explained by solar extreme ultraviolet heating alone. Our analysis yields one heat source peaking at ∼1 × 10-5 μbar (range 8 × 10-7-2 × 10-5 micro;bar) with an integrated heating rate of approximately 0.06 (+0.02, -0.04) erg cm-2 sec-1 as the least-squares best fit to all occultation data. The best inferred temperature for the stellar entrance occultation (63.7° S) is at least 50 K cooler near 50 μbar than for the stellar exit occultation (69.7° N), whereas at about 0.1 μbar this temperature contrast is less than 10 K. A constant temperature on pressure surfaces at low altitudes, however, cannot be excluded by the data." @default.
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- W2075492634 date "1993-01-01" @default.
- W2075492634 modified "2023-09-28" @default.
- W2075492634 title "An Analysis of the Voyager 2 Ultraviolet Spectrometer Occultation Data at Uranus: Inferring Heat Sources and Model Atmospheres" @default.
- W2075492634 doi "https://doi.org/10.1006/icar.1993.1005" @default.
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