Sunspot continuum from 1 to 10 microns and the umbral temperature models

Details Sunspot continuum from 1 to 10 microns and the umbral temperature models Sunspot continuum from 1 to 10 microns and the umbral temperature models

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984basi...12..233p&link_type=abstract

Astronomical Society of India, Bulletin, vol. 12, Sept. 1984, p. 233-236.

Astronomy and Astrophysics

Astronomy

Haze, Infrared Astronomy, Solar Temperature, Sunspots, Umbras, M Stars, Molecular Spectra, Opacity, Photosphere, Solar Observatories

Scientific paper

The molecular-line haze-opacity correction of Joshi et al. (1979) is applied in computing the 1-10-micron IR flux of sunspots for the models of Zwaan (1974) and Boyer (1980). The results are presented in a graph and a table and compared to the 1-2.1-micron flux observations of Sitnik (1980). It is found that the model temperatures for both models need to be increased to make them agree with the observations, but that the opacity correction does not remove discrepancies between the models.

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