Abstract
First results of the campaign to measure the OI 630.0 nm dayglow emission continuously from an equatorial station, Sriharikota (5.5° dip latitude), India, during January–February 1989 are presented. Results from zenith observations during five days reveal close coupling with the F-region electron densities controlled by the electrodynamical processes, showing features like the noon-time ‘bite-outs’ and several other fine features. These new results give us clues for identifying the significant processes that result in OI 630.0 nm dayglow emission.
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