P. D. Angreji
Articles written in Journal of Astrophysics and Astronomy
Volume 3 Issue 1 March 1982 pp 69-77
Fabry-Perot interferometric observations on the green coronal line (λ 5303 å) carried out during the total solar eclipse of 1980 February 16 have yielded relative Doppler shift velocities with an accuracy of ± 7 km s-1. The values show a peak in the 30–50 km s-1 range indicating largescale macroscopic mass motion in the solar maximum corona.
Volume 41, 2020
Continuous Article Publishing mode
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