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THE EXTREME ULTRAVIOLET SPECTRUM OF HIGHLY CHARGED COPPER IONS

Journal Article · · Astronomical Journal (Online)
;  [1]; ;  [2];  [3]
  1. Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou (China)
  2. Department of Nuclear Physics, China Institute of Atomic Energy, Beijing (China)
  3. College of Physics and Electronic Engineering, Northwest Normal University, Lanzhou (China)
This paper reports the laboratory measurements of extreme ultraviolet spectra of highly charged copper ions. In this work, 82 lines from Cu xv to Cu xxiii in the 160–360 Å wavelength range are identified as the transitions of the 2p{sup 2}3p–2p{sup 2}3d, 2p{sup 4}3s–2p{sup 4}3p, 2p{sup 4}3p–2p{sup 4}3d, 2p{sup 5}3s–2p{sup 5}3p, 2p{sup 5}3s–2p{sup 5}3p, 3s3p–3p{sup 2}, 3s{sup 2}3p{sup 3}-3s3p{sup 4}, 3s{sup 2}3p–3s3p{sup 2}, 3s{sup 2}3p{sup 3}–3s3p{sup 4}, and 2p{sup 4} ({sup 3}P)3s–2p{sup 4} ({sup 3}P) 3p, in which 40 spectral lines have been newly and accurately measured. Their identification is based on comparisons with available experimental and theoretical values and the calculations with Cowan codes.
OSTI ID:
22662941
Journal Information:
Astronomical Journal (Online), Journal Name: Astronomical Journal (Online) Journal Issue: 5 Vol. 152; ISSN 1538-3881
Country of Publication:
United States
Language:
English

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