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- W3104131473 abstract "At wavelengths between 0.15 and 0.19 $mu$m, the far-ultraviolet spectrum of Jupiter is dominated by the scattered solar spectrum, attenuated by molecular absorptions primarily by acetylene and ethane, and to a lesser extent ammonia and phosphine. We describe the development of our radiative transfer code that enables the retrieval of abundances of these molecular species from ultraviolet reflectance spectra. As a proof-of-concept we present an analysis of Cassini Ultraviolet Imaging Spectrograph (UVIS) observations of the disk of Jupiter during the 2000/2001 flyby. The ultraviolet-retrieved acetylene abundances in the upper stratosphere are lower than those predicted by models based solely on infrared thermal emission from the mid-stratosphere observed by the Composite Infrared Spectrometer (CIRS), requiring an adjustment to the vertical profiles above 1 mbar. We produce a vertical acetylene abundance profile that is compatible with both CIRS and UVIS, with reduced abundances at pressures $<$1 mbar: the 0.1 mbar abundances are $1.21 pm 0.07$ ppm for acetylene and $20.8 pm 5.1$ ppm for ethane. Finally, we perform a sensitivity study for the JUICE UVS instrument, which has extended wavelength coverage out to 0.21 $mu$m, enabling the retrieval of ammonia and phosphine abundances, in addition to acetylene and ethane." @default.
- W3104131473 created "2020-11-23" @default.
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- W3104131473 date "2020-06-03" @default.
- W3104131473 modified "2023-10-14" @default.
- W3104131473 title "Jupiter in the Ultraviolet: Acetylene and Ethane Abundances in the Stratosphere of Jupiter from Cassini Observations between 0.15 and 0.19 <i>μ</i>m" @default.
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- W3104131473 doi "https://doi.org/10.3847/1538-3881/ab91a6" @default.
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