Probable additional Swan band lines in the solar spectrum

Details Probable additional Swan band lines in the solar spectrum Probable additional Swan band lines in the solar spectrum

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985basi...13..127s&link_type=abstract

Astronomical Society of India, Bulletin, vol. 13, June 1985, p. 127-130.

Astronomy and Astrophysics

Astronomy

1

Solar Spectra, Swan Bands, Carbon, Spectral Line Width

Scientific paper

A study of the identification of the (0-0) band of the Swan system of the C2 molecules in the wavelength region 4800-5200 A is presented. The C2 wavelengths of Phillips and Davis (1968) are compared with the line identifications of Moore et al. (1966). The equivalent widths of the lines are calculated for the center of the solar disc and for a near limb position using the photospheric model of Holweger and Mueller (1974). A table of calculated equivalent widths and equivalent widths measured by Moore et al. (1966) is provided.

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