Fig. 10From: Planetary-scale MLT waves diagnosed through multi-station methods: a reviewAdjusted Feynman diagrams of interactions between Rossby-gravity waves ([\(\frac{1}{50h}\),3],[\(\frac{1}{41h}\),4]) and four migrating components: a [1cpd,1]–[\(\frac{1}{50h}\),3], b [1cpd,1]+[\(\frac{1}{50h}\),3], c [2cpd,2]–[\(\frac{1}{50h}\),3], d [2cpd,2]+[\(\frac{1}{50h}\),3], e [3cpd,3]–[\(\frac{1}{50h}\),3], f [1cpd,1]–[\(\frac{1}{41h}\),4], g [2cpd,2]+[\(\frac{1}{41h}\),4], h [3cpd,3]–[\(\frac{1}{41h}\),4], i [4cpd,4]–[\(\frac{1}{41h}\),4]Back to article page