Theoretical intensity ratios for the X-ray lines from CA XV

Details Theoretical intensity ratios for the X-ray lines from CA XV Theoretical intensity ratios for the X-ray lines from CA XV

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...155..417b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 155, no. 2, Feb. 1986, p. 417-419. DOE-SERC-supported research.

Astronomy and Astrophysics

Astronomy

3

Line Spectra, Solar Spectra, Solar X-Rays, X Ray Astronomy, Atomic Spectra, Calcium, Electron Scattering, Solar Flares

Scientific paper

Electron collision strengths for Ca XV have been obtained using the 'distorted wave' approximation. Previous results (Mason, 1975; Dere et al., 1979) were obtained for the configurations 2s22p2, 2s2p3, 2p4. The authors present results for transitions 2s22p2 → 2s22p3s, 2s22p3d which give rise to lines in the X-ray spectra of solar active regions and flares.

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