Wavelength Measurements of Ni L-shell Lines between 9 and 15 A

Details Wavelength Measurements of Ni L-shell Lines between 9 and 15 A Wavelength Measurements of Ni L-shell Lines between 9 and 15 A

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006head....9.1836g&link_type=abstract

American Astronomical Society, HEAD meeting #9, #18.36; Bulletin of the American Astronomical Society, Vol. 38, p.387

Astronomy and Astrophysics

Astronomy

Scientific paper

We present accurate wavelength measurements of nikel L-shell X-ray lines resulting from Δ n ≥ 1 transitions (mostly, 2 - 3 transitions) between 9 and 15 Å. We have used the electron beam ion trap, SuperEBIT, at the Lawrence Livermore National Laboratory and a flat field grating spectrometer to record the spectra. Most significant emission lines of Ni XIX -- XXVI in our spectral coverage are identified. The resulting data set provides valuable input in the analyses of high resolution X-ray spectra of stellar coronae sources, including the Sun.
This work was performed under the auspices of U.S. DOE contract No. W-7405-Eng-48, and supported by NASA APRA Grant NAG5-5419.

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