Comparison of satellite spectra for H-like Fe and He-like Fe, Ca, and S calculated by three different methods

Atomic Data and Nuclear Data Tables

Volumn 67, Issue 2, 1997, Pages 225-329

  Kato, Takako ^a   Safronova, Ulyana I ^b   Shlyaptseva, Alla S ^b   Cornille, Marguerite ^c   Dubau, Jacques ^c   Nilsen, Joseph ^d  

^a NATIONAL INSTITUTE FOR FUSION SCIENCE   (Japan)

^b INSTITUTE OF SPECTROSCOPY   (Russian Federation)

^c OBSERVATOIRE DE PARIS   (France)

^d LAWRENCE LIVERMORE NATIONAL LABORATORY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

C (PROGRAMMING LANGUAGE);

EXPANSION METHODS; INNER SHELL; MODEL POTENTIAL; SATELLITE LINES; SATELLITE SPECTRA; SOLAR FLARE; SPECTRA'S; STATISTIC MODELING; SYNTHETIC SPECTRA; THEORETICAL ATOMIC DATA;

SATELLITES;

EID: 0031281179     PISSN: 0092640X     EISSN: None     Source Type: Journal    
DOI: 10.1006/adnd.1997.0752     Document Type: Article

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