Solar X-Ray Spectrum below 25 Angstroms

Details Solar X-Ray Spectrum below 25 Angstroms Solar X-Ray Spectrum below 25 Angstroms

Nov 1964

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1964sci...146.1037b&link_type=abstract

Science, Volume 146, Issue 3647, pp. 1037-1038

Physics

3

Scientific paper

Below 25 angstrom, 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.

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