Solar line blocking for disk-center and disk-averaged radiation from 3300 to 6860 A

Details Solar line blocking for disk-center and disk-averaged radiation from 3300 to 6860 A Solar line blocking for disk-center and disk-averaged radiation from 3300 to 6860 A

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...95..229n&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 95, Feb. 1985, p. 229-238.

Physics

6

Solar Radiation, Solar Spectra, Blocking, Fourier Transformation, Line Spectra, Spectral Bands, Ultraviolet Spectra, Visible Spectrum

Scientific paper

The line blocking is tabulated for 10 Å (λ < 6300 Å) or 20 Å (λ > 6300 Å) wide intervals. It follows from the spectral averages and the local continuum derived by Neckel and Labs from high-resolution Fourier transform spectra, which had been obtained by J. Brault at Kitt Peak. The internal accuracy (the scatter) is in the order of 0.1%. Significant systematic errors arising from local distortions of the adopted continuum level can be excluded. Larger errors are to be expected only near the Balmer limit where the localization of the "continuum" is very ambiguous.

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