Physics
Scientific paper
May 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979colo.reptq....g&link_type=abstract
Annual Report, 15 Apr. 1978 - 15 May 1979 Denver Univ., CO. Dept. of Physics.
Physics
Gases, Light (Visible Radiation), Solar Spectra, Ultraviolet Spectra, Absorption Spectra, Absorptivity, Graphs (Charts), Nitrogen Oxides, Ozone, Simulation, Solar Radiation
Scientific paper
The data compiled during the study allowed a detailed examination of the attenuation of the solar radiance by the combined effect of the atmospheric trace gases and the SAGE filters. The case of the 0.44 microns channel is presented. The amounts of NO2, NO2, O3 and the airmass were chosen to closely simulate a low sun spectral scan from a 9 February 1977 balloon flight. The solar radiance outside the earth's atmosphere was determined from the AFGL Sacramento Peak Observatory spectral data tape degraded to 2.0A resolution and normalized to Thekaekara's absolute intensities. The spectral absorption coefficients used for NO2 and O3 were tabulated previously.
No associations
LandOfFree
Theoretical simulation of solar spectra in the middle ultraviolet and visible for atmospheric trace constituent measurements does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Theoretical simulation of solar spectra in the middle ultraviolet and visible for atmospheric trace constituent measurements, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Theoretical simulation of solar spectra in the middle ultraviolet and visible for atmospheric trace constituent measurements will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1702119