Fig. 23
Power distributions for different H I phases at − 8 < vLSR < 8 km s−1. Top left: WNM; top right: LNM; bottom left: CNM; and bottom right: sum of all phases with uncertainties from the Gaussian decomposition (cyan and orange). Black lines show all-sky data; red lines are for |b| > 20°. Spectral indices γ for CNM, LNM, and CNM are derived at 10 < l < 100 for the sum of all phases at l > 8, as indicated by the vertical lines.
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