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• W2000911918 abstract "[1] The Hopkins Ultraviolet Telescope (HUT) was one of three ultraviolet Astro-1 observatory instruments on space shuttle Columbia in December 1990 (STS-35), covering the 830–1850 Å wavelength interval (first order) at ∼3.3 Å spectral resolution. Satellite altitude was 360 km. Dayside nadir measurements were performed during a single orbit on 7 December 1990 under solar maximum (F10.7 = 222), geomagnetically quiet (Ap = 4) conditions, covering late morning local times (solar zenith angle < 48°). These data constitute a reference dayglow radiance spectrum comprising a number of thermospheric emission features, including several weak features neighboring bright optically thick emissions, that have not yet received adequate explanations, in part owing to questions regarding spectral intensity calibration, dynamic range, etc., associated with older data sets. In this paper, the HUT extreme ultraviolet (EUV)–far ultraviolet (FUV) nadir dayglow spectrum is presented along with the results of a modeling analysis using a development version of the Atmospheric Ultraviolet Radiance Integrated Code (AURIC). The analysis relies on currently available laboratory data and first-principles excitation and transport modeling codes and utilizes constraints drawn from the FUV spectral region data to study several EUV emissions of interest for which past airglow data are sparse. The focus is on the airglow in the 980–1200 Å region, which is particularly rich in emission features affected by thermospheric conditions. Emissions investigated in detail include (1) the optically thick OI 989 Å multiplet and associated 1172 Å fluorescence, (2) the OI 1026 Å sextuplet blended with atomic hydrogen Lyman β, (3) the atomic nitrogen multiplets at 1134 and 1200 Å consisting of optically thick components excited by e− + N and optically thin components excited by e− + N2 and hν + N2, (4) a number of other NI and N+ features (e.g., N+ 1085 Å) excited by N2 dissociative ionization, (5) the Birge-Hopfield I (N2 BH-1) system, and (6) the resonance lines of argon (Ar 1048 and 1067 Å)." @default.
• W2000911918 created "2016-06-24" @default.
• W2000911918 creator A5002868421 @default.
• W2000911918 creator A5010120800 @default.
• W2000911918 date "2003-01-01" @default.
• W2000911918 modified "2023-10-14" @default.
• W2000911918 title "Analysis of the Astro-1/Hopkins Ultraviolet Telescope EUV–FUV dayside nadir spectral radiance measurements" @default.
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• W2000911918 doi "https://doi.org/10.1029/2001ja000330" @default.
• W2000911918 hasPublicationYear "2003" @default.
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