Other
Scientific paper
Jan 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apjs...54..167t&link_type=abstract
Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 54, Jan. 1984, p. 167-175.
Other
32
Solar Spectra, Spectral Energy Distribution, Stellar Spectrophotometry, Ubv Spectra, Balmer Series, Stellar Color
Scientific paper
New spectrophotometry for 12 solar-type stars providing virtually complete wavelength coverage between 3288 and 7000 A is reported. Instrumental colors are calculated from the solar irradiance, stellar flux curves, and adopted response functions and are transformed to the UBV system by using observed stellar colors. The resulting solar colors agree well with previously published exact counterparts. Comparison of the irradiance curves for the sun and a similar star reveals no evidence of systematic error in the Balmer-confluence region of the parent stellar flux curves. Transformation equations from this procedure appear to reproduce the UBV system for solar-type stars quite closely. Solar colors are reported for five published irradiance curves and are compared to other photometric solar colors from the literature. Indirect techniques yield solar (B-V) in the range 0.60-0.66.
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