Doppler width of CH lines

Details Doppler width of CH lines Doppler width of CH lines

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.181..327p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 181, no. 2, July 1991, p. 327-329.

Astronomy and Astrophysics

Astrophysics

Doppler Effect, Hydrocarbons, Solar Spectra, Spectral Line Width, Fourier Transformation, Line Spectra, Solar Flux

Scientific paper

Twenty-one CH line profiles at the center of the solar disk were
Fourier-transformed to derive the Doppler widths. The Doppler width
increases linearly with the equivalent width.

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