E. A. Makarova
Articles written in Journal of Astrophysics and Astronomy
Volume 9 Issue 1 March 1988 pp 41-47
Using the line profiles of [Fe x] 6374 å and [Fe XIV] 5303 å emission lines observed during five total solar eclipses, we address the problem whether the solar corona is static or contains moving features. Many of the profiles of both emission lines have complicated shapes, which we interpret as an evidence for the existence of many, small, moving features in the corona. The line-of-sight velocities observed by other investigators (
Volume 9 Issue 2 June 1988 pp 125-125 Erratum
Volume 40 | Issue 3
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