Solar EUV line identifications from delayed beam-foil spectra

Details Solar EUV line identifications from delayed beam-foil spectra Solar EUV line identifications from delayed beam-foil spectra

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998mnras.297..399t&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 297, Issue 2, pp. 399-404.

Astronomy and Astrophysics

Astronomy

21

Atomic Data, Line Identification, Sun: Corona

Scientific paper

A number of electric dipole transitions from low-lying long-lived levels
in Si-, P- and S-like ions of Fe and neighbouring elements have been
identified by their longevity in delayed EUV spectra after foil
excitation of fast ion beams. Some of these new identifications pertain
to previously unidentified lines in solar flare spectra.

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