CO fluorescence in the extreme-ultraviolet solar spectrum

Details CO fluorescence in the extreme-ultraviolet solar spectrum CO fluorescence in the extreme-ultraviolet solar spectrum

Jul 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...223l..51b&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 223, July 1, 1978, p. L51-L53.

Astronomy and Astrophysics

Astrophysics

20

Carbon Monoxide, Chromosphere, Solar Spectra, Sunspots, Ultraviolet Spectra, High Resolution, Opacity, Solar Limb, Spectral Resolution, Spectrum Analysis, Sun

Scientific paper

Emission lines in the fourth positive system of CO have been identified in the extreme-ultraviolet solar spectrum 1540-1660 A. These lines are excited by the C IV transition-zone lines at 1548 and 1551 A. They are strong in the spectrum of a sunspot and in parts of the adjacent active region. Some of them appear as weak, broad emission features in the quiet sun.

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