NE VII emission lines in the solar EUV spectrum

Details NE VII emission lines in the solar EUV spectrum NE VII emission lines in the solar EUV spectrum

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999soph..186..231m&link_type=abstract

Solar Physics, v. 186, Issue 1/2, p. 231-242 (1999).

Physics

Scientific paper

Recent calculations of electron and proton impact excitation rates in Nevii are used to calculate theoretical emission line ratios involving both Deltan=0 (2-2) and Deltan=1 (2-3) transitions in the ~97-895Å wavelength range. A comparison of these with existing solar observations, obtained by instruments on rocket flights and on the Skylab mission, reveals generally good agreement between theory and observation. This provides experimental support for the accuracy of the atomic data adopted in the line ratio calculations, and implies that the latter may be applied with confidence to the analysis of solar and stellar spectra from current and future satellite missions.

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