THEORETICAL XUV SPECTRA FROM CARBON-LIKE COBALT IONS BY RELATIVISTIC CONFIGURATION INTERACTION CALCULATION
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Abstract
Allowed Δn = 0 transitions of highly ionized metal atoms, which may appear in the solar spectra as well as in spectra from the high-temperature tokamak plasmas, lie in the extreme vacuum UV (XUV) region, 100Å≤ λ ≤ 200Å . Here we report our theoretical calculation of the Δn = 0 transitions of C-like cobalt ions; it is in good agreement with the experimental measurement. Such theoretical calculations of the transition wave lengths and their oscillator strengths should be very helpful to identify the XUV spectra.
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ZOU Yu, LI Jiaming. THEORETICAL XUV SPECTRA FROM CARBON-LIKE COBALT IONS BY RELATIVISTIC CONFIGURATION INTERACTION CALCULATION[J]. Chin. Phys. Lett., 1990, 7(5): 216-218.
ZOU Yu, LI Jiaming. THEORETICAL XUV SPECTRA FROM CARBON-LIKE COBALT IONS BY RELATIVISTIC CONFIGURATION INTERACTION CALCULATION[J]. Chin. Phys. Lett., 1990, 7(5): 216-218.
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ZOU Yu, LI Jiaming. THEORETICAL XUV SPECTRA FROM CARBON-LIKE COBALT IONS BY RELATIVISTIC CONFIGURATION INTERACTION CALCULATION[J]. Chin. Phys. Lett., 1990, 7(5): 216-218.
ZOU Yu, LI Jiaming. THEORETICAL XUV SPECTRA FROM CARBON-LIKE COBALT IONS BY RELATIVISTIC CONFIGURATION INTERACTION CALCULATION[J]. Chin. Phys. Lett., 1990, 7(5): 216-218.
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