The problem of the energy distribution in the solar spectrum

Details The problem of the energy distribution in the solar spectrum The problem of the energy distribution in the solar spectrum

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989azh....66..583m&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 66, May-June 1989, p. 583-595. In Russian.

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4

Solar Spectra, Spectral Energy Distribution, Color, G Stars, Illuminance, Stellar Spectrophotometry

Scientific paper

The energy distribution in the solar spectrum in the 255-1060 nm range is obtained as a weighted average of the most reliable measurements. The reliability of each series of measurements was examined using an objective criterion. This involves a comparison between the color indices in the 13-color Johnson-Mitchell system calculated for one or another energy distribution in the solar spectrum and the normal indices of solar-type stars.

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