Observations in the Mojave Desert of the diurnal variations of the zenith intensity of the forbidden oxygen line at 5577 A for ten nights over a two-year interval are recorded. In general, a maximum of intensity occurs at local midnight, ±2.5 hours. A detailed study of one night is reported wherein the diurnal variation of regions of the sky other than the zenith are shown to follow time patterns similar in general but with significant variations in detail. The intensity changes of various parts of the sky are interpreted as geographical variations of local zenith intensity. Isophotal plots of these geographical variations throughout the night indicate the presence of definite patterns in the upper atmosphere. During the post-twilight period, an enhancement of intensity is observed in the western sky. In the predawn observations, no enhancement is noted in the eastern sky. Between the post-twilight and predawn, the intensity goes through a maximum which is partially localized to the north of our station. Evidence is presented which indicates that the over-all intensity change can be described as a fixed excitation pattern on the dark side of the earth through which a given observer seems to move with the rotation of the earth. The character of the pattern seems to change with the season. The variation of intensity with zenith distance for the whole night indicates an effective height of emission of 250 km.
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