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• W2018561190 abstract "Limb scans of nighttime sodium doublet emissions at 589 nm were performed globally from a Sun‐synchronous satellite during July 1979. The observations have provided a global description of variation in the emitting layer with latitude and altitude. The limb scan data are consistent with the presence of a 10‐km‐thick emitting layer near the 90‐km peak of the sodium density in the northern mid‐latitude mesosphere in summer. At equatorial and southern latitudes, however, a narrower emission layer occurs 5–10 km lower, and the intensity is stronger by a factor of 3 or more. It appears likely that the shape of the Na D emission profile is influenced by the altitude distributions of both sodium and ozone, the reactants which are necessary to produce the emission. The observed variability may be explained by a systematic seasonal mismatch in the altitude of the mesospheric density maxima for sodium and ozone, combined with a known threefold wintertime increase in sodium density." @default.
• W2018561190 created "2016-06-24" @default.
• W2018561190 creator A5012284646 @default.
• W2018561190 date "1988-05-01" @default.
• W2018561190 modified "2023-10-14" @default.
• W2018561190 title "Nighttime Na<i>D</i>emission observed from a polar-orbiting DMSP satellite" @default.
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• W2018561190 doi "https://doi.org/10.1029/ja093ia05p04067" @default.
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