Published April 1995
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Comparison of the satellite lines of H-like and He-like spectra
Description
The two kinds of theoretical atomic data by MZ method with Z expansion (Vainshtein and Safronova (1978)) and AUTOLSJ method with intermediate coupling (Dubau et al (1981), TFR group et al (1981)) for the wavelengths and the dielectronic and inner shell satellite lines of H-like ions and He-like Fe, Ca and S ions are compared in a form of the synthetic spectra. The agreement is rather good within 20% for main satellite lines. (author)
Availability note (English)
MF available from INIS under the Report Number.
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Additional details
Publishing Information
- Imprint Pagination
- 134 p.
- Report number
- NIFS-DATA--24
INIS
- Country of Publication
- Japan
- Country of Input or Organization
- Japan
- INIS RN
- 26075040
- Subject category
- S74: ATOMIC AND MOLECULAR PHYSICS;
- Descriptors DEI
- CALCIUM IONS; ENERGY-LEVEL TRANSITIONS; HELIUM IONS; HYDROGEN IONS; INNER-SHELL EXCITATION; IRON IONS; SULFUR IONS; WAVELENGTHS; X-RAY SPECTRA
- Descriptors DEC
- CHARGED PARTICLES; EXCITATION; IONS; SPECTRA