Physics
Scientific paper
Feb 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...90..205n&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 90, Feb. 1984, p. 205-258.
Physics
365
Infrared Spectra, Solar Radiation, Solar Spectra, Spectral Energy Distribution, Visible Spectrum, Black Body Radiation, Calibrating, Error Analysis, Fourier Transformation, Irradiance, Spectral Bands, Telluric Lines
Scientific paper
The results are based on absolute measurements of the disk-center intensities made more than 20 years ago and on Fourier transform spectra. A homogeneous and consistent set of absolute radiation data with high internal accuracy is derived for these FTS spectra. With a standard deviation of less than 0.2 percent, the maximum errors to be expected are of the order of 0.5 percent. This value is also seen as the upper limit for a neutral scale error, which may affect the overall irradiance integral (solar constant), and for systematic deviations occurring in relatively short spectral regions owing to the limited accuracy of the calibration curves. It is pointed out, however, that the overall spectral distribution cannot be seriously affected by systematic errors. This conclusion derives from the fact that the solar irradiance distribution agrees within observational errors with the flux distributions observed by Hardorp (1980) for solar-type stars (Neckel and Labs, 1981).
Labs Dietrich
Neckel Heinz
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