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28 September 1999 Far-ultraviolet stellar occultation measurements of the upper atmosphere
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We describe the analysis methods of the stellar occultation measurement technique, and present preliminary results of upper atmospheric measurements with Princeton University's Interstellar Medium Absorption Profile Spectrometer (IMAPS), which was flown on two Shuttle AstroSPAS missions. The primary objective of IMAPS was to study the interstellar medium, but it also made observations of some hot stars as they were occulted by Earth's upper atmosphere. These observations provided the first detailed measurements of upper atmospheric O and N2 by the stellar occultation method. We also present a conceptual design for a follow-on instrument, dedicated to stellar occultation measurements of the upper atmosphere, the Global Upper Atmospheric Neutral Density from Stellar Occultations investigation.
© (1999) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
George R. Carruthers and Edward B. Jenkins "Far-ultraviolet stellar occultation measurements of the upper atmosphere", Proc. SPIE 3818, Ultraviolet Atmospheric and Space Remote Sensing: Methods and Instrumentation II, (28 September 1999);

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