Correction to “Latitudinal and seasonal models of stratospheric photochemistry on Saturn: Comparison with infrared data from IRTF/TEXES”

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Errata

This article corrects:

  1. Latitudinal and seasonal models of stratospheric photochemistry on Saturn: Comparison with infrared data from IRTF/TEXES Volume 110, Issue E9, Article first published online: 20 September 2005

[1] In the paper “Latitudinal and seasonal models of stratospheric photochemistry on Saturn: Comparison with infrared data from IRTF/TEXES” by J. I. Moses and T. K. Greathouse (Journal of Geophysical Research, 110, E09007, doi:10.1029/2005JE002450), owing to a publisher's error, an incorrect version of Figure 10 was presented. The correct version of Figure 10 is presented here.

Figure 10.

The model-derived mixing-ratio profiles of the observed constituents (a) CH4, (b) CH3, (c) C2H2, (d) C2H4, (e) C2H6, (f) CH3C2H, (g) C3H8, (h) C4H2, (i) C6H6, and (j) H as a function of latitude for Ls = 273° (southern summer, northern winter, January 2003). The dashed lines represent −8°, the solid lines represent −36°, the dot-dashed lines represent −69°, the dotted lines represent 32° latitude, and the triple-dot-dashed lines represent 80° latitude.

Figure 10.

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