Jupiter's Atmospheric Composition from the Cassini Thermal Infrared Spectroscopy Experiment

@article{Kunde2004JupitersAC,
  title={Jupiter's Atmospheric Composition from the Cassini Thermal Infrared Spectroscopy Experiment},
  author={V. G. Kunde and F. Flasar and D. Jennings and B. B'ezard and D. Strobel and B. Conrath and C. Nixon and G. Bjoraker and P. Romani and R. Achterberg and A. Simon-Miller and P. Irwin and J. Brasunas and J. Pearl and M. Smith and G. Orton and P. Gierasch and L. Spilker and R. Carlson and A. Mamoutkine and S. Calcutt and P. Read and F. W. Taylor and T. Fouchet and P. Parrish and A. Barucci and R. Courtin and A. Coustenis and D. Gautier and E. Lellouch and A. Marten and R. Prang{\'e} and Y. Biraud and C. Ferrari and T. Owen and Mian M. Abbas and R. E. Samuelson and F. Raulin and P. Ade and C. Cesarsky and K. Grossman and A. Coradini},
  journal={Science},
  year={2004},
  volume={305},
  pages={1582 - 1586}
}
  • V. G. Kunde, F. Flasar, +39 authors A. Coradini
  • Published 2004
  • Medicine, Chemistry
  • Science
  • 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… CONTINUE READING

    Topics from this paper.

    Composite infrared spectrometer (CIRS) on Cassini.
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    Modelling the near-infrared spectra of Jupiter using line-by-line methods
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    References

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