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Phys. Rev. A 63, 022710 (2001) [11 pages]

Dielectronic satellite contributions to Ne VIII and Ne IX K-shell spectra

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B. J. Wargelin* and S. M. Kahn
Department of Physics and Space Sciences Laboratory, University of California, Berkeley, California 94720

P. Beiersdorfer
Lawrence Livermore National Laboratory, 7000 East Avenue, Livermore, California 94550

Received 8 August 2000; published 17 January 2001

Kα spectra of heliumlike neon and associated lithiumlike, berylliumlike, and boronlike satellite line emission have been observed with a high-resolution crystal spectrometer on the Lawrence Livermore Electron Beam Ion Trap. The KLL dielectronic recombination satellites were resolved from their He-like parent lines in electron energy space, and their wavelengths and resonance strengths measured. The wavelength measurements achieved a typical accuracy of a few mÅ, with two measurements accurate to better than one part in 10 000. By normalizing to the He-like resonance line, w, we measure Li-like satellite resonance strengths that are 10% to 46% lower than predicted by theoretical models. The wavelengths and relative strengths of Be-like KLL satellites were also measured, and absolute strengths were obtained by normalizing to the collisionally excited Li-like qr satellite blend.

© 2001 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevA.63.022710
DOI:
10.1103/PhysRevA.63.022710
PACS:
32.80.Hd, 32.30.Rj, 32.70.Fw, 34.80.Kw

*Present address: Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138.

Present address: Department of Physics, Columbia University, 538 West 120th Street, New York, NY 10027.