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dc.creatorBell, E. E.en_US
dc.creatorEisner, I. L.en_US
dc.date.accessioned2006-06-15T12:50:04Z
dc.date.available2006-06-15T12:50:04Z
dc.date.issued1957en_US
dc.identifier1957-E-5en_US
dc.identifier.urihttp://hdl.handle.net/1811/7620
dc.description$^{*}$This work was done under contract between Wright Air Development Center and The Ohio State University Research Foundation. $^{1}$Butler, NRL Report 3981, June, 1952. $^{2}$Oetjen, Bell, Young, Metter, J. Opt. Soc. Am. 45, 403 (1955). $^{3}$Sloan, Shaw, and Williams, J. Opt. Soc. Am. 45, 445 (1955). $^{4}$Burch and Shaw. J. Opt. Soc. Am. 47, 227 (1957).en_US
dc.descriptionAuthor Institution: The Ohio State Universityen_US
dc.description.abstract“Data will be presented to show the measured spectral radiance of the sky (0$^\circ K$ reference temperature) in the one to twenty microns wavelength region. The relative importance of atmospheric $emission^{1,2,3,4}$ and scattered sunlight will be shown. The importance of the temperature, water vapor content, altitude, sun angle, elevation, and azimuth will be illustrated with typical spectra. A semi-quantitative explanation of the effects of these variables will be given on the basis of a simple model of the atmosphere.”en_US
dc.format.extent71603 bytes
dc.format.mimetypeimage/jpeg
dc.language.isoenen_US
dc.publisherOhio State Universityen_US
dc.titleINFRARED RADIATION FROM THE $SKY^{*}$en_US
dc.typearticleen_US


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