J. A. Pirraglia

TL;DR: During the passage of Voyager 1 through the Saturn system, the infrared instrument acquired spectral and radiometric data on Saturn, the rings, and Titan and other satellites, implying a depletion of helium in the atmosphere of Saturn relative to that of Jupiter.

TL;DR: In this article, spectral features due to the atmospheric dust storm indicate that large diurnal variations in atmospheric temperature existed up to at least 30 km; winds inferred from the temperature fields show a strong tidal component and significant ageostrophic behavior.

TL;DR: The infrared spectroscopy and radiometry investigation has obtained spectra of Jupiter and its satellites between approximately 180 and 2500 cm–1 with a spectral resolution of 4.3cm–1, showing clear evidence of H2, CH4 C2H2, C2 H6, CH3D, NH3, PH3, H2O, and GeH4.

TL;DR: In this paper, a low-resolution pressure map is presented which covers that portion of the planet between latitudes -60 deg and +25 deg, and a more detailed study of the Coprates canyon indicates that at its lowest point the canyon floor must be at least 5 km below the rim.

TL;DR: During the passage of Voyager 2 through the Saturn system, infrared spectral and radiometric data were obtained for Saturn, Titan, Enceladus, Tethys, Iapetus, and the rings, suggesting an approximate symmetry in the small-scale structure.