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Measurements of rocket spectrograms obtained from Aerobee-Hi flights on June 4, 1958, and March 30, 1959, have yielded wave lengths of about 150 solar ultraviolet emission lines in the range between 1216 (HLa) and 83.9 A. Estimates of the intensity of the He ii 303.8 A line were made. Measured wave lengths corrected for systematic errors and, in some cases, identifications of the lines are given.
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Violett et al. (1959) studied this question.
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