Contours of the relative difference between the deep temperature in the non-grey model and in the semi-grey model for different values of γv in function of the width of the lines and their strength. The non-grey atmosphere is 10% hotter (resp. cooler) than the semi-grey atmosphere inside the red (resp. blue) contours. The dashed lines are contours of γP. We used μ∗ = 1/.
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