Article ID Journal Published Year Pages File Type
10705261 Planetary and Space Science 2012 8 Pages PDF
Abstract
► Saturn haze 3-μm absorption feature is retrieved from Cassini/VIMS occultation data. ► It's spectral structure is modeled with absorption by condensated hydrocarbons. ► Possible formation processes of these ices in Saturn's atmosphere are discussed.
Keywords
Related Topics
Physical Sciences and Engineering Earth and Planetary Sciences Geophysics
Preview
The three-micron spectral feature of the Saturnian haze: Implications for the haze composition and formation process
Authors
, , , , , ,