The solar minimum temperature determined by the CO (A 1 Pi - X 1 Sigma)

Details The solar minimum temperature determined by the CO (A 1 Pi - X 1 Sigma) The solar minimum temperature determined by the CO (A 1 Pi - X 1 Sigma)

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.116..165m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 116, no. 1, Nov. 1985, p. 165-172.

Astronomy and Astrophysics

Astrophysics

Carbon Monoxide, Solar Spectra, Solar Temperature, Atmospheric Temperature, Electron Transitions, Emission Spectra, Franck-Condon Principle, Minima, Molecular Rotation, Vibrational Spectra

Scientific paper

The synthetic Voigt profiles of the following transitions (υarcsec = 0, υarcmin = 0), (υarcsec = 0, υarcmin = 1), (υarcsec = 1, υarcmin = 1), (υarcsec = 1, υarcmin = 0) have been computed for different concentrations and temperatures of CO and compared to the measured intensities of the UV sunspot spectrum by a high resolution spectrograph. From this comparison the solar minimum temperature has been determined.

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