Wavelength Measurements of Ni L-Shell Lines between 9 and 15 Å

Astronomy and Astrophysics – Astronomy

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Atomic Data, Line: Identification, Stars: Coronae, Sun: Corona, Sun: X-Rays, Gamma Rays, X-Rays: General

Scientific paper

We present accurate wavelength measurements of nickel L-shell X-ray lines resulting from Δn>=1 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. The most significant emission lines of Ni XIX-XXVI in our spectral coverage are identified, and their relative intensities are determined. The resulting data set provides valuable input for the analyses of high-resolution X-ray spectra of stellar coronae sources, including the Sun.

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