Fe XXIII-Fe XIX theoretical spectra in two calculational methods
1988
Two different calculational methods are compared for atomic data used to analyse transitions of the type 1s2sk2pn-1s22sk2pn-1. Wavelengths, radiative transitions, autoionisation probabilities and intensity factors are compared. These parameters are needed for diagnostics of low-density plasmas as found in solar flares and tokamak devices.
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