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Fig. 3
First gravity modes (0 ≤ n ≤ 5) of normalized Hough functions 
, 
, and 
corresponding to the semidiurnal tide of Venus-like exoplanets (m = 2 and ν = 0.4804). We note that ν = 2Ω /σ. For more details about the behaviour of Hough functions, see Figs. A.2.
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