Space Ultraviolet Spectroscopy and Imaging of Jupiter

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Hopkins Ultraviolet Telescope, Hubble Space Telescope

Scientific paper

We have observed Jupiter in the ultraviolet band of wavelengths from 850-1850 A using the Hopkins Ultraviolet Telescope, the Hubble Space Telescope, and a sounding rocket experiment. These measurements comprise moderate-resolution equatorial and north polar spectra and images that probe the stratosphere of Jupiter. We have determined that the abundances of acetylene, ethane and ethylene were 39 ± 3 ppb, 3 ± 1 ppm and <0.4 ppb respectively in 1990, and 28 ± 3 ppb, 3 ± 1 ppm and 0.4 ± 0.2 ppb in 1995. The integrated (1450-1850 A) contribution of the H2 dayglow was 800 ± 400 Rayleighs in 1990 and <400 Rayleighs in 1995, which was a period spanning solar maximum and solar minimum. The polar data have shown the molecular hydrogen aurora to extend over 4.5±0.5×10-10 sr with an average brightness of 106 ± 12 kR integrated over the band of wavelengths from 900 to 1650 A, excluding Lyα. We measure a 13% larger emitting area (5.1±0.5×10-10 sr) and significantly different morphology for the combined atomic and molecular hydrogen aurora (Lyα + H2), although these differences could be due to time variability. Color ratios derived from the data indicate a total auroral energy deposition rate of 13 ergs s-1/ cm-2 by 3-30 keV electrons. The sounding rocket development program has involved parallel studies of CCD detectors and ultraviolet spectrographs. These studies have included characterization of front and back-illuminated UV-sensitive CCDs with average quantum efficiencies of 18% and 40%, respectively, and the development of an aberrationless LiF prism spectrograph for imaging of UV astronomical targets.

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