Spectral line parameters for the pure rotation bands of solar OH

Details Spectral line parameters for the pure rotation bands of solar OH Spectral line parameters for the pure rotation bands of solar OH

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983jqsrt..29..469g&link_type=abstract

Journal of Quantitative Spectroscopy and Radiative Transfer (ISSN 0022-4073), vol. 29, May 1983, p. 469, 470. NSF-supported rese

Physics

14

Hydroxyl Radicals, Molecular Rotation, Photosphere, Solar Spectra, Spectral Line Width, Electron Transitions, Parameterization, Solar Atmosphere

Scientific paper

Spectral line parameters for the Δυ = 0 rotation transitions
of OH observable in the solar photosphere are generated. The line
parameters, which include line positions, ground state energies and
intensities, are calculated at 6000K for the X2Π (0-0),
(1-1), (2-2), and (3-3) bands.

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