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Fig. 5.

image

Upper left: power spectra of ffast as a function of height and frequency for the BATT run. For better visualization, the maps are scaled with a factor of ρ0, the density of the unperturbed atmosphere. The power is shown in log10 units of J m−5 Hz−1. Upper right panels: ratio of power between the AMBI and BATT, AMBIHALL and BATT, and AMBIHALL and AMBI runs. Contours mark the locations where the power ratio is unity. Bottom panels: same, but for falf.

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