SIMULTANEOUS OBSERVATIONS OF SODIUM DENSITY AND THE NAD, OH (8, 3), AND OI 5577-A NIGHTGLOW EMISSIONS

Simultaneous observations of the vertical distribution of sodium density and the intensities of the OI 5577-A, NaD, and OH (8, 3) airglow emissions show that the nocturnal variations of the emissions are well correlated with those of the sodium at 91, 87, and 84 km, respectively. In the case of NaD and OH (8, 3) these heights correspond closely to expected heights of peak airglow emission, although in the case of OI 5577 A, maximum emission would be expected from about 4 km higher. The correlated variations appear to be caused by atmospheric waves having vertical wavelengths between 10 and 15 km whose phases propagate downward with velocities between 1 and 2 km/hr** minus **1. The amplitude of the correlated nocturnal variations in sodium density on the bottom side of the layer is normally too large to be explained as the direct result of atmospheric density changes. These large variations could be the result of vertical motions of the layer or might be caused by changes in the equilibrium between sodium and its oxide.