Fourier transform spectrometer observations of solar carbon monoxide. II - Simultaneous cospatial measurements of the fundamental and first-overtone bands, and CA II K, in quiet and active regions

Astronomy and Astrophysics – Astronomy

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Atmospheric Composition, Carbon Monoxide, Molecular Spectra, Solar Atmosphere, Solar Spectra, Brightness Temperature, Chromosphere, Infrared Astronomy, K Lines, Photosphere, Solar Limb, Solar Spectrometers, Spectral Bands

Scientific paper

Fourier transform spectrometry has yielded simultaneous cospatial measurements of important diagnostics of thermal structure in the high solar photosphere and low chromosphere. It is noted that the anomalous behavior of the fundamental bands of CO in quiet areas near the limb is accentuated in an active region plage observed close to the limb. The difference between the core temperatures of the CO fundamental bands in a plage and a nearby quiet region at the limb is larger than the corresponding brightness temperature differences in the inner wings of the Ca II line measured in a quiet region and several plages closer to the disk center. Numerical simulations indicate that the disparate behavior of the CO bands with respect to Ca II K cannot be reconciled with existing single component thermal structure models; a two-component atmosphere is required.

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