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Analysis of the spatial distribution of dayside cleft optical emissions

Journal Article · · J. Geophys. Res.; (United States)
OSTI ID:5019274
An analysis of measurements of the 4278-A, 5200-A, 5577-A and 6300 A emissions obtained from a rocket launch through the postnoon dayside cleft into the polar cap ionosphere is reported. The 4278-A and 5577-A emission show a clearly defined decrease in intensity at the poleward edge of the dayside particle precipatation, while the 5200-A emission extends well into the polar cap with only a slight decrease in intensity. The 6300-A emission displays a behavior intermediate between these extremes. The optical data are analyzed by using a dynamical model of dayside cleft auroral processes incorporating transport by ion and neutral winds. It is concluded that neutral winds are responsible for modifying the spatial distribution of the 5200-A and 6300-A emission while the ion drift component is negligible. In addition, it is found that (1) 80% of the 4278-A emission intensity is due to resonance fluorescence in the sunlit cleft ionosphere, (2) the reaction O/sub 2/(c/sup 1/..sigma../sub u//sup -/)+O..-->.. O/sub 2/+O(/sup 1/S) is consistent with the 5577-A data if the yield of O(/sup 1/S) from the dissociative recombination of O/sub 2//sup +/ is about 2%, and (3) the rate of the reaction N/sub 2//sup +/+O..-->..NO/sup +/+N is apparently higher in the ionosphere than indicated by the laboratory measurements.
Research Organization:
Centre for Research in Experimental Space Science, York University
OSTI ID:
5019274
Journal Information:
J. Geophys. Res.; (United States), Journal Name: J. Geophys. Res.; (United States) Vol. 88:A12; ISSN JGREA
Country of Publication:
United States
Language:
English