Skip to main content
Fig. 4 | Earth, Planets and Space

Fig. 4

From: Cloud trains associated with Martian Mountain Lee Waves on the eastern side of the Phlegra Montes

Fig. 4

The seasonal variabilities in the number of cloud trains and the background atmospheric variables. a The number of cloud trains, b water ice mixing ratio, c zonal wind, and d atmospheric temperature in the target area, WAP, are displayed. The gray bars in Panel a indicate the number of the MOC blue images available for this study. The blue, green, and red bars indicate the numbers of detected cloud trains whose wavelengths are short, middle, and long, respectively. The variables shown in Panels b, c, and d are derived from the EMARS 1.0 and interpolated into the pressure coordinate

Back to article page