Abstract
This paper reviews solar extreme ultraviolet observations made in the spectral region λ170 — λ400 by the first Orbiting Solar Observatory during March, April, and May, 1962. Application of the data to the identification of emission lines in this spectral region is discussed. The observations are compared with concurrent 2800 MHz radio emission and other measurements of solar activity.
Publisher
Cambridge University Press (CUP)
Cited by
2 articles.
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