On 5694 A coronal line observations

Physics

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Coronagraphs, Light (Visible Radiation), Line Spectra, Solar Corona, Solar Spectra, Angular Distribution, Emission Spectra, Luminous Intensity

Scientific paper

Continuous emission in the 5694 A yellow coronal line was observed on January 17 and 28, 1971 and on August 21, 1972 with a Lyot coronagraph, using a curved slit. The lines 6374 A and 5303 A were photographed in the yellow line emission region, and the intensity distribution in these lines is plotted against the position angle. A decrease in 6374 and 5303 A line intensity is observed in the yellow line emission region.

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