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We review the observational evidence that the warm ionized medium (WIM) is amajor and physically distinct component of the Galactic interstellar medium.Although up to ~20% of the faint, high-latitude H-alpha emission in the MilkyWay may be scattered light emitted in midplane H II regions, recent scatteredlight models do not effectively challenge the well-established properties ofthe WIM.

Modern view of the warm ionized medium