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Fig. 4 | Earth, Planets and Space

Fig. 4

From: Evaluation of a method to retrieve temperature and wind velocity profiles of the Venusian nightside mesosphere from mid-infrared CO2 absorption line observed by heterodyne spectroscopy

Fig. 4

Standard deviations for the a temperature and b wind velocity in the retrieval results from five model spectra shown in Fig. 1. The meaning of the colored lines is the same as that in Fig. 1. Green lines (VIRAex case) in a and b are the same as the black dashed lines in Figs. 2b and 3, respectively

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