Results are presented, which follow from the merging of: (a) our previously published absolute integrals of the disk-center intensity for 20 Å wide spectral bands; (b) the ratios of mean to central intensity derived from recent observations of the center-to-limb variation of those bands (λ <6600 Å); (c) the ratios of mean to central intensity derived from the observations of the center-to-limb variation at continuum-wavelengths according to Pierce and Slaughter (λ >6600 Å); (d) the high resolution Fourier transform spectra obtained by J. Brault at Kitt Peak for the disk-center and the irradiance; (e) some further auxiliary data, which served mainly to eliminate the local perturbations caused by lines of telluric molecular bands.The main result is the presentation of high precision radiation data for both the integrated disk and the disk-center, concerning the line-averaged radiation and the continuum (in UV: highest ‘window’-intensities) as well.The internal accuracy (the ‘scatter’) should not be worse than that of the FTS spectra, which is less than 0.2% (mean error); local systematic deviations exceeding 0.5% are not to be expected. The absence of a significant systematic error - neutral or wavelength-dependent - has been proven already elsewhere.
[1]
A. K. Pierce,et al.
Relative Solar Energy Distribution in the Spectral Region 10,000-25,000 a.
,
1954
.
[2]
H. Neckel,et al.
Transformation of the absolute solar radiation data into the ‘International Practical Temperature Scale of 1968’
,
1970
.
[3]
A. Broadfoot.
The Solar Spectrum 2100-3200 Å
,
1972
.
[4]
A. V. Kharitonov,et al.
Distribution of energy in the solar spectrum and the solar constant
,
1974
.
[5]
P. Simon,et al.
Solar flux determination in the spectral range 150–210 nm
,
1976
.
[6]
A. K. Pierce,et al.
Solar limb darkening
,
1977
.
[7]
O. White.
The Solar Output and Its Variation
,
1977
.
[8]
D. Weinberger,et al.
Solar limb darkening in the interval 7404-24 018 Å, II
,
1977
.
[9]
H. Neckel,et al.
Improved data of solar spectral irradiance from 0.33 to 1.25 microns
,
1981
.
[10]
C. Fröhlich,et al.
Solar radiation and its variation in time
,
1981
.
[11]
F. Frey,et al.
Geochemical characteristics of boninite series volcanics: implications for their source
,
1982
.