Paper
22 January 1993 Horizon UV Program (HUP) atmospheric radiance measurements
Francis J. LeBlanc, F. P. DelGreco, J. A. Welsh, Robert E. Huffman
Author Affiliations +
Abstract
Spectrometric observations (1100 A to 1800 A) of the ultraviolet radiance of Earth's atmosphere have been obtained by the Horizon Ultraviolet Program (HUP) sensor from Space Shuttle altitude at two different points in the solar cycle. Most of the radiance measurements were made during horizon scans of the earthlimb or while the HUP field of view was directed toward nadir. The expected variation of dayglow radiance with solar zenith angle (SZA) in the several spectral bands was observed. These results compare favorably to the predictions of a preliminary version of the Atmospheric Ultraviolet Radiance Integrated Code (AURIC).
© (1993) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Francis J. LeBlanc, F. P. DelGreco, J. A. Welsh, and Robert E. Huffman "Horizon UV Program (HUP) atmospheric radiance measurements", Proc. SPIE 1764, Ultraviolet Technology IV, (22 January 1993); https://doi.org/10.1117/12.140850
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KEYWORDS
Ultraviolet radiation

Data modeling

Oxygen

Earth's atmosphere

Atmospheric modeling

Sensors

Spectroscopy

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