The wavelength dependence of the facular excess brightness

Details The wavelength dependence of the facular excess brightness The wavelength dependence of the facular excess brightness

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...217..657c&link_type=abstract

Astrophysical Journal, Part 1, vol. 217, Oct. 15, 1977, p. 657-660. Research supported by the Aerospace Corp.

Other

22

Brightness, Colorimetry, Faculae, Photosphere, Stellar Spectrophotometry, Stellar Structure, Oblate Spheroids, Relativity, Solar Limb, Wavelengths

Scientific paper

Observations are presented of the wavelength dependence of photospheric solar faculae obtained during August 1975. Systematic observations with an extreme limb photometer were carried out in five different bands. Plots of the limb brightness of a facular region for each of the five colors are presented in a graph. Another graph shows the wavelength dependence of the facular excess brightness, normalized to unity for the green filter used. The wavelength variation to be expected from the facular contribution to oblateness measurements is listed in a table.

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