Doppler width of CN lines in the sun

Details Doppler width of CN lines in the sun Doppler width of CN lines in the sun

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984basi...12..393p&link_type=abstract

Astronomical Society of India, Bulletin, vol. 12, Dec. 1984, p. 393-397.

Astronomy and Astrophysics

Astronomy

2

Cyanogen, Doppler Effect, Solar Spectra, Spectral Line Width, Solar Atmosphere, Vibrational Spectra

Scientific paper

The Doppler widths of the lines of the CN violet system have been determined in the 4139-4215 A wavelength region in the solar atmosphere. The profile fitting, saturation effects, and depth of line formation are discussed. The results show that the lines of the 0-1 band form higher and of the 2-3 band lower down in the solar atmosphere. The Doppler widths of the 0-1, 1-2, and 2-3 bands increase linearly with equivalent widths up to roughly 20 mA.

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