Distribution of HCN (solid line) compared with the profile obtained by Vinatier et al. (2007) from Cassini/CIRS data at 15°S latitude (dotted line) and by Courtin et al. (2011) from Herschel/SPIRE data (short dashes). Long-dashed lines show the 1-σ limit. The curves in the small box represent the weighting functions for each line. We used the same line order as in Fig. 5 (from left to right).
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