Line blocking in the solar spectrum

Details Line blocking in the solar spectrum Line blocking in the solar spectrum

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975a%26a....45...19a&link_type=abstract

Astronomy and Astrophysics, vol. 45, no. 1, Dec. 1975, p. 19-24.

Astronomy and Astrophysics

Astrophysics

9

Absorption Spectra, Atmospheric Attenuation, Solar Spectra, Telluric Lines, Astronomical Catalogs, Astronomical Photometry, Brightness Temperature, Continuous Spectra, Late Stars, Light (Visible Radiation), Luminous Intensity

Scientific paper

Solar line-blocking coefficients for the wavelength region between 4300 and 6200 A are derived from observational data contained in a recent photometric atlas of the solar spectrum. The technique for defining the solar continuum is outlined, apparent blocking coefficients are determined for 10-A intervals, and intrinsic blocking coefficients are obtained by reducing the apparent values for effects of telluric absorption lines. The results are compared with those of several previous studies of line blocking in the solar spectrum.

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