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

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 and Z. Pujic

Nature, 2008, vol. 451, issue 7181, 1022-1022

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).

Date: 2008
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DOI: 10.1038/nature06807

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