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dc.creatorWark, D. Q.en_US
dc.date.accessioned2006-06-15T13:36:42Z
dc.date.available2006-06-15T13:36:42Z
dc.date.issued1975en_US
dc.identifier1975-ME-08en_US
dc.identifier.urihttp://hdl.handle.net/1811/9258
dc.descriptionAuthor Institution: NOAA,, National Environmental Satellite Serviceen_US
dc.description.abstractMeasurements of the solar intensity by the University of Denver scanning spectrometer were made during a balloon ascent to 40 km on 3 December 1974. Spectral resolution was 0.01 $\mu$m. A filter radiometer measured the sun continuously in the 11 $\mu m$ window. Combining the radiometer output with a spectral scan of a hot laboratory source and published solar spectral radiances provides a 100\% level, which is tested against the spectrometer data in the wings of the band at the higher altitudes. Spectral transmittance versus pressure for the solar zenith angle during the ascent will be used as a standard for the general computation of atmospheric transmittances to be used with satellite data for indirect sounding of atmospheric temperature.en_US
dc.format.extent106233 bytes
dc.format.mimetypeimage/jpeg
dc.language.isoEnglishen_US
dc.publisherOhio State Universityen_US
dc.titleMEASUREMENT TO 40 km OF ATMOSPHERIC TRANSMITTANCES IN THE 15 $\mu m$ BAND OF CARBON DIOXIDEen_US
dc.typearticleen_US


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