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Erratum: Depth of a strong jovian jet from a planetary-scale disturbance driven by storms

Author

Listed:
  • A. Sánchez-Lavega
  • G. S. Orton
  • R. Hueso
  • E. García-Melendo
  • S. Pérez-Hoyos
  • A. Simon-Miller
  • J. F. Rojas
  • J. M. Gómez
  • P. Yanamandra-Fisher
  • L. Fletcher
  • J. Joels
  • J. Kemerer
  • J. Hora
  • E. Karkoschka
  • I. de Pater
  • M. H. Wong
  • P. S. Marcus
  • N. Pinilla-Alonso
  • F. Carvalho
  • C. Go
  • D. Parker
  • M. Salway
  • M. Valimberti
  • A. Wesley
  • Z. Pujic

Abstract

Nature 451, 437–440 (2008) In Fig. 3a, the descriptions of the continuous and dotted curves were inadvertently swapped. The continuous line corresponds to the modified synthetic thermal profile (storms reaching the 60 mbar level). The dotted line corresponds to the Cassini CIRS thermal profile (storms reaching the 160 mbar level).

Suggested Citation

  • A. Sánchez-Lavega & G. S. Orton & R. Hueso & E. García-Melendo & S. Pérez-Hoyos & A. Simon-Miller & J. F. Rojas & J. M. Gómez & P. Yanamandra-Fisher & L. Fletcher & J. Joels & J. Kemerer & J. Hora & E, 2008. "Erratum: Depth of a strong jovian jet from a planetary-scale disturbance driven by storms," Nature, Nature, vol. 451(7181), pages 1022-1022, February.
  • Handle: RePEc:nat:nature:v:451:y:2008:i:7181:d:10.1038_nature06807
    DOI: 10.1038/nature06807
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