Molecular line haze opacity in sunspots

Details Molecular line haze opacity in sunspots Molecular line haze opacity in sunspots

May 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979soph...62...83g&link_type=abstract

Solar Physics, vol. 62, May 1979, p. 83-87.

Physics

6

Haze, Line Spectra, Molecular Spectra, Opacity, Sunspots, Transition Flow, Abundance, Calcium Compounds, Carbon Compounds, Hydrides, Hydrogen Ions, Infrared Spectra, Magnesium Compounds, Nitrites, Solar Physics, Titanium Oxides, Umbras

Scientific paper

This paper demonstrates that bound-bound opacity due to electronic transitions of the molecules CN, CaH, MgH, and TiO largely explains, in the first approximation, the line haze opacity postulated by Zwaan (1974) for the wavelength region from 0.5 to 0.9 micron in the umbral spectrum. Relative umbral intensities in the cited wavelength region are calculated and compared with observations. The computed relative intensities are shown to agree fairly well with those obtained by Zwaan for an additional component of continuous opacity.

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