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- W1515709631 abstract "The French instrument on board OSO-8 is a multichannel, high resolution (0.02 Å) UV spectrometer, observing very small solar areas (from 1″ x 1″ of arc to 6″ x 2′ of arc) simultaneously in the Ca II, Mg II, Ly α, Ly β lines. Using a classical inversion technique as described by Roble and Hays (1972) it has been possible to invert some extinction profiles. The quality of the data appears to give a 500 m vertical resolution both for O3 and O2. O3 is essentially observed from 55 to 75 km and O2 from 85 to 200 km. Due to the velocity of the spectral scan mechanism (able to scan Ly a line in 2.56 s) it was possible to observe the differential extinction of the Lyman alpha line when absorbed by O2. Furthermore data on the atomic hydrogen absorption give a new method of evaluating the exospheric temperature and atomic hydrogen density at each point of the exobase." @default.
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- W1515709631 date "1976-01-01" @default.
- W1515709631 modified "2023-09-27" @default.
- W1515709631 title "High Resolution Atmospheric Extinction Measurements from the French Experiment on Board the NASA Spacecraft OSO-8" @default.
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- W1515709631 doi "https://doi.org/10.1007/978-94-010-1528-8_9" @default.
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