Intensity Dependence of the Asymmetry of Fraunhofer Line Profiles

Details Intensity Dependence of the Asymmetry of Fraunhofer Line Profiles Intensity Dependence of the Asymmetry of Fraunhofer Line Profiles

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001arep...45...75k&link_type=abstract

Astronomy Reports, Volume 45, Issue 1, January 2001, pp.75-78

Astronomy and Astrophysics

Astronomy

Scientific paper

The integral, residual, and relative asymmetries of the profiles of 120 weak and medium-strength Fraunhofer lines in the spectrum of the central solar disk are determined. The digitized spectral materials used were obtained using rapid-scanning, high-dispersion double monochromators. The integral profile asymmetries grow appreciably with line equivalent width, while the residual and relative profile asymmetries do not show such a strong dependence.

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