Solar X-Ray Spectrum below 25 Angstroms
- 20 November 1964
- journal article
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 146 (3647) , 1037-1038
- https://doi.org/10.1126/science.146.3647.1037
Abstract
Below 25 Å, the solar spectrum consists primarily of the emission lines of Fe XVII, O VIII, O VII, and N VII. The lines of the more highly ionized atoms, Fe XVII and O VIII, originate in localized active regions. Lines of O VII and N VII emanate from the full disk.Keywords
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