FIGURE 2. Vertical–zonal map of ethane abundance.
From the following article:
An equatorial oscillation in Saturn's middle atmosphere
T. Fouchet, S. Guerlet, D. F. Strobel, A. A. Simon-Miller, B. Bézard & F. M. Flasar
Nature 453, 200-202(8 May 2008)
doi:10.1038/nature06912

This pressure–latitude cross-section of the ethane volume mixing ratio (indicated by the contours) is inverted by fitting the v9-band of ethane (820 cm-1) observed by the CIRS between 1 and 0.01 hPa. The temperature field used in the calculation is presented in Fig. 1. CIRS spectra measuring the temperature and the composition were obtained simultaneously at the same vertical and spectral resolution. Vertical profiles of the ethane volume mixing ratio were retrieved by means of a constrained inversion with strong low-pass filtering (see Supplementary Information).
