2017
DOI: 10.1002/2017gl074014
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WINDII airglow observations of wave superposition and the possible association with historical “bright nights”

Abstract: Longitudinal variations of airglow emission rate are prominent in all midlatitude nighttime O(1S) lower thermospheric data obtained with the Wind Imaging Interferometer (WINDII) on the Upper Atmosphere Research Satellite (UARS). The pattern generally appears as a combination of zonal waves 1, 2, 3, and 4 whose phases propagate at different rates. Sudden localized enhancements of 2 to 4 days duration are sometimes evident, reaching vertically integrated emission rates of 400 R, a factor of 10 higher than minimu… Show more

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Cited by 10 publications
(7 citation statements)
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“…First, airglow itself is highly variable. In addition to long-term variations that are related to the solar cycle [12], airglow also changes with the seasons [13], and even on quite short time scales [14]. Second, satellite sensors with a wide swath observe Earth at variable nadir angles θ n .…”
Section: Introductionmentioning
confidence: 99%
“…First, airglow itself is highly variable. In addition to long-term variations that are related to the solar cycle [12], airglow also changes with the seasons [13], and even on quite short time scales [14]. Second, satellite sensors with a wide swath observe Earth at variable nadir angles θ n .…”
Section: Introductionmentioning
confidence: 99%
“…Satellite observations suggest historical bright nights are the result of zonal wave superposition. 7 Walker, Krisciunas, and others have correlated observed variations in night sky brightness with prior changes in EUV from the Sun as measured by the 10.7cm (2.8 GHz) solar flux5,6. The hypothesis is, changes in photoionization on the Earth's day-side produce subsequent variable night time airglow by re-radiation from atoms and molecules in a complex chemical environment.…”
Section: Articlementioning
confidence: 90%
“…Rose (35) obtained a visual sensation with 100 photons • s −1 . Using an 8 mm pupil for the eye and 2 arcmin for a pixel, it can be calculated that the photon flux required to stimulate a physical sensation is 200 Rayleigh (36). Under the same illumination condition, only a brightness greater than 200 Rayleigh can be perceived by the eye at other wavelengths.…”
Section: Methodsmentioning
confidence: 99%