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

Research output: Contribution to journalArticle

Abstract

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 (
Original languageEnglish
JournalAmerican Astronomical Society, DPS meeting #50
Volume39
Publication statusPublished - 1 Oct 2007
Externally publishedYes

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Saturn
spectrometer
hydrocarbon
upper atmosphere
Southern Hemisphere
climate modeling
temporal variation
temperature

Cite this

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.
Hesman, Brigette E. ; Jennings, D. E. ; Sada, P. V. ; Bjoraker, G. L. ; Simon-Miller, A. A. ; Nixon, C. A. ; Boyle, R. J. ; McCabe, G. H. / Saturn's Hydrocarbon Emission from Ground-based and Cassini/CIRS Observations. In: American Astronomical Society, DPS meeting #50. 2007 ; Vol. 39.
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Hesman, BE, Jennings, DE, Sada, PV, Bjoraker, GL, Simon-Miller, AA, Nixon, CA, Boyle, RJ & McCabe, GH 2007, 'Saturn's Hydrocarbon Emission from Ground-based and Cassini/CIRS Observations', American Astronomical Society, DPS meeting #50, vol. 39.

Saturn's Hydrocarbon Emission from Ground-based and Cassini/CIRS Observations. / Hesman, Brigette E.; Jennings, D. E.; Sada, P. V.; Bjoraker, G. L.; Simon-Miller, A. A.; Nixon, C. A.; Boyle, R. J.; McCabe, G. H.

In: American Astronomical Society, DPS meeting #50, Vol. 39, 01.10.2007.

Research output: Contribution to journalArticle

TY - JOUR

T1 - Saturn's Hydrocarbon Emission from Ground-based and Cassini/CIRS Observations

AU - Hesman, Brigette E.

AU - Jennings, D. E.

AU - Sada, P. V.

AU - Bjoraker, G. L.

AU - Simon-Miller, A. A.

AU - Nixon, C. A.

AU - Boyle, R. J.

AU - McCabe, G. H.

PY - 2007/10/1

Y1 - 2007/10/1

N2 - 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 (

AB - 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 (

M3 - Article

VL - 39

JO - American Astronomical Society, DPS meeting #50

JF - American Astronomical Society, DPS meeting #50

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Hesman BE, Jennings DE, Sada PV, Bjoraker GL, Simon-Miller AA, Nixon CA et al. Saturn's Hydrocarbon Emission from Ground-based and Cassini/CIRS Observations. American Astronomical Society, DPS meeting #50. 2007 Oct 1;39.