Computer Science – Sound
Scientific paper
Dec 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989spie.1158..319d&link_type=abstract
IN: Ultraviolet technology III; Proceedings of the Meeting, San Diego, CA, Aug. 10, 11, 1989 (A90-43258 19-35). Bellingham, WA,
Computer Science
Sound
Atmospheric Effects, Cassegrain Optics, Stellar Luminosity, Ultraviolet Photography, Ultraviolet Telescopes, Atmospheric Composition, Atmospheric Sounding, Earth Atmosphere, Ultraviolet Astronomy
Scientific paper
An 18-in Cassegrain telescope and UV imaging system is used to observe and record starlight in the wavelength range 3000-3700 A. The spatial dependence for the transmission of radiation through the atmosphere has been calculated using the LOWTRAN 6 computer code, and the results are compared to data from various UV-emitting stars. Variations in the atmosphere are seen to strongly depend on aerosol concentration which affects meteorological range. Ground-level photometer measurements of extinction coefficients are extrapolated to yield atmospheric visibility profiles for the observation point.
Baisley V. C.
Dentamaro Anthony V.
Stergis Christos G.
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