Tidal and Solar Cycle Effects on the OI 5577 Angstrom, NaD and OH(8,3)Airglow Emissions Observed at 23 Deg S

摘要

The upper mesosphere airglow emissions OI 5577, NaD and OH were observed at Cachoeira Paulista (22.7 S; 45.0 W) Brazil. Nocturnal variations and their seasonal dependencies in amplitude and phase, and the annual variations of these emissions are presented, analyzing the data obtained from 1977 to 1982 during the ascending phase of the last solar cycle. The nocturnal variations of the OI 5577 emission and the OH rotational temperature showed a significant semidiurnal oscillation, with the phase of maximum moving from the midnight in January to early morning in June. Semiannual variation of the OI 5577 and NaD emissions with the maximum intensities in April/May and October/November were observed. The OH rotational temperature, however, showed an annual variation, maximum in summer and minimum in winter, while no significant seasonal variation was found in the OH emission intensities. Long term intensity variations are also presented with the solar sunspot numbers and the 10.7 cm flux.