Saturn's Hydrocarbon Emission from Ground-based and Cassini/CIRS Observations

Brigette E. Hesman, D. E. Jennings, P. V. Sada, G. L. Bjoraker, A. A. Simon-Miller, C. A. Nixon, R. J. Boyle, G. H. McCabe

Resultados de investigaciones

Resumen

Hydrocarbons in the upper atmosphere of Saturn are known, from Voyager and early Cassini results, to vary in emission intensity with latitude. Of particular interest is the marked increase in temperature and hydrocarbon line intensity near the South Pole (Greathouse et al. 2005, Orton and Yanamandra-Fisher, 2005, Flasar et al. 2005). Latitudinal variations in hydrocarbon abundances can be determined from measurements of hydrocarbon emission lines using temperatures derived from Cassini's Composite InfraRed Spectrometer (CIRS). Latitudinal, temporal, and vertical variations of stratospheric hydrocarbons provide constraints on dynamics, seasonal climate models, and photochemical models. In an effort to monitor temporal and latitudinal variations of hydrocarbons in Saturn's southern hemisphere we are conducting a ground-based campaign using Celeste, an infrared (5-25 μm) high-resolution (
Idioma originalEnglish
RevistaAmerican Astronomical Society, DPS meeting #50
Volumen39
Estado de la publicaciónPublished - 1 oct 2007
Publicado externamente

    Huella digital

Citar esto

Hesman, B. E., Jennings, D. E., Sada, P. V., Bjoraker, G. L., Simon-Miller, A. A., Nixon, C. A., ... McCabe, G. H. (2007). Saturn's Hydrocarbon Emission from Ground-based and Cassini/CIRS Observations. American Astronomical Society, DPS meeting #50, 39.