Skip to main content
Earth, Planets and Space
Fig. 3 | Earth, Planets and Space

Fig. 3

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. 3

Retrieved wind velocity profiles from the model spectrum generated from temperature of VIRAex and wind velocity of 0 m/s (green line in Fig. 1). Colored lines show the profiles retrieved with 41 a priori wind velocity profiles (red: positive wind velocity, blue: negative wind velocity). Black dashed line shows the standard deviation for these profiles

Back to article page