Abstract
Spectra obtained during the May 30, 1965 eclipse by Dunn aboard the NASA aircraft are presented and analyzed. Equivalent widths and absolute intensities are given for 39 coronal lines between 3300 and 8200 A around the west limb of the Sun at two heights. Details are given on the reduction process, and comparisons are made with other observations from the same eclipse. Some line identifications are discussed.
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