Investigation of wave characteristics by red coronal line observations

S. I. Molodykh, N. F. Tyagun
2004 Proceedings of the International Astronomical Union  
This paper presents the results of the active region observations in red coronal line (λ = 6374 • A). The analysis was made of the dependence of the profile parameters of the red coronal line on the exposition value.
doi:10.1017/s1743921304007185 fatcat:53n4lbpfd5hnbegqv4orvbyehi