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DOI10.1126/science.1100240
Jupiter's atmospheric composition from the Cassini thermal infrared spectroscopy expirement
Kunde V.G.; Flasar F.M.; Jennings D.E.; Bézard B.; Strobel D.F.; Conrath B.J.; Nixon C.A.; Bjoraker G.L.; Romani P.N.; Achterberg R.K.; Simon-Miller A.A.; Irwin P.; Brasunas J.C.; Pearl J.C.; Smith M.D.; Orton G.S.; Gierasch P.J.; Spilker L.J.; Carlson R.C.; Mamoutkine A.A.; Calcutt S.B.; Read P.L.; Taylor F.W.; Fouchet T.; Parrish P.; Barucci A.; Courtin R.; Coustenis A.; Gautier D.; Lellouch E.; Marten A.; Prangé R.; Biraud Y.; Ferrari C.; Owen T.C.; Abbas M.M.; Samuelson R.E.; Raulin F.; Ade P.; Césarsky C.J.; Grossman K.U.; Coradini A.
发表日期2004
ISSN0036-8075
起始页码1582
结束页码1586
卷号305期号:5690
英文摘要The Composite Infrared Spectrometer observed Jupiter in the thermal infrared during the swing-by of the Cassini spacecraft. Results include the detection of two new stratospheric species, the methyl radical and diacetylene, gaseous species present in the north and south auroral infrared hot spots; determination of the variations with latitude of acetylene and ethane, the latter a tracer of atmospheric motion; observations of unexpected spatial distributions of carbon dioxide and hydrogen cyanide, both considered to be products of comet Shoemaker-Levy 9 impacts; characterization of the morphology of the auroral infrared hot spot acetylene emission; and a new evaluation of the energetics of the northern auroral infrared hot spot.
英文关键词Acetylene; Atmospherics; Carbon dioxide; Ethane; Morphology; Spacecraft; Upper atmosphere; Hydrogen cyanide; Thermal infrared spectroscopy; Infrared spectroscopy; acetylene; acetylene derivative; carbon dioxide; diacetylene; ethane; hydrogen cyanide; methyl group; radical; unclassified drug; carbon dioxide; hydrocarbon; hydrogen cyanide; infrared spectroscopy; Jupiter; planetary atmosphere; article; astronomy; atmosphere; chemical composition; energy transfer; evaluation; gas analysis; infrared spectroscopy; latitude; parameter; precipitation; prediction; priority journal; space flight; stratosphere; atmosphere; microclimate; spectroscopy; temperature; Acetylene; Atmosphere; Carbon Dioxide; Ethane; Extraterrestrial Environment; Hydrocarbons; Hydrogen Cyanide; Jupiter; Spacecraft; Spectrum Analysis; Temperature
语种英语
来源期刊Science
文献类型期刊论文
条目标识符http://gcip.llas.ac.cn/handle/2XKMVOVA/244424
作者单位Department of Astronomy, University of Maryland, College Park, MD 20742, United States; NASA/Goddard Space Flight Center, Code 693, Greenbelt, MD 20771, United States; LESIA, CNRS-UMR8109, Observatoire de Paris, 5 place Jules Janssen, F-91925 Meudon Cedex, France; Johns Hopkins University, Dept. of Earth and Planetary Science, Baltimore, MD 21218, United States; Department of Astronomy, Cornell University, Ithaca, NY 14853, United States; Space Science and Applications, Inc., 5900 Princess Garden Parkway, Lanham, MD 20706, United States; Atmospheric, Oceanic/Planet. Phys., Clarendon Laboratory, University of Oxford, Parks Road, Oxford OX1 3PU, United Kingdom; Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, United States; CEA Saclay, Service d'Astrophysique, 91191 Gif-sur-Yvette Cedex, France; University of Hawaii, Institute of Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822, United States; NASA/Marshall Space Flight Center, Huntsville, AL 35812, United States; LISA, Université de P...
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Kunde V.G.,Flasar F.M.,Jennings D.E.,et al. Jupiter's atmospheric composition from the Cassini thermal infrared spectroscopy expirement[J],2004,305(5690).
APA Kunde V.G..,Flasar F.M..,Jennings D.E..,Bézard B..,Strobel D.F..,...&Coradini A..(2004).Jupiter's atmospheric composition from the Cassini thermal infrared spectroscopy expirement.Science,305(5690).
MLA Kunde V.G.,et al."Jupiter's atmospheric composition from the Cassini thermal infrared spectroscopy expirement".Science 305.5690(2004).
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