Centre-to-limb behaviour of molecular rotational temperatures. III

Details Centre-to-limb behaviour of molecular rotational temperatures. III Centre-to-limb behaviour of molecular rotational temperatures. III

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984basi...12..172s&link_type=abstract

Astronomical Society of India, Bulletin, vol. 12, June 1984, p. 172-181.

Astronomy and Astrophysics

Astronomy

8

Molecular Rotation, Solar Atmosphere, Solar Limb, Solar Spectra, Atmospheric Models, Line Spectra, Swan Bands

Scientific paper

The rotational temperatures of the (0-0) band of the Swan system of C(2) molecules at mu = 1.0 and 0.2 are calculated using solar-observation data from the KPNO atlas of Brault and Testerman (1972). The results are presented in tables and graphs and compared with those obtained with the model atmospheres of Holweger and Mueller (1974) and Vernazza et al. (1976). Good agreement is found at the solar-disk center, but the model temperatures tend to be lower than the observation-based temperatures near the limb. No evidence is found for the temperature increase toward the limb reported by Sinha (1979) on the basis of the observational data of Withbroe (1968).

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