Study of X-ray photoionized Fe plasma and comparisons with astrophysical modeling codes

Journal of Quantitative Spectroscopy and Radiative Transfer

Volumn 99, Issue 1-3, 2006, Pages 712-729

  Foord, M E ^a   Heeter, R F ^a   Chung, H K ^a   van Hoof, P A M ^c   Bailey, J E ^b   Cuneo, M E ^b   Liedahl, D A ^a   Fournier, K B ^a   Jonauskas, V ^c   Kisielius, R ^c   Ramsbottom, C ^c   Springer, P T ^a   Keenan, F P ^c   Rose, S J ^d   Goldstein, W H ^a  

^a LAWRENCE LIVERMORE NATIONAL LABORATORY   (United States)

^b SANDIA NATIONAL LABORATORIES   (United States)

^c QUEEN'S UNIVERSITY BELFAST   (United Kingdom)

^d UNIVERSITY OF OXFORD   (United Kingdom)

Author keywords

Astrophysical observation; Plasma spectroscopy; Population kinetics; X ray spectra

Indexed keywords

ABSORPTION SPECTROSCOPY; APPROXIMATION THEORY; ASTROPHYSICS; COMPUTER SIMULATION; MATHEMATICAL MODELS; OPACITY; PHOTOIONIZATION; X RAY SPECTROSCOPY;

ASTROPHYSICAL OBSERVATION; PLASMA SPECTROSCOPY; POPULATION KINETICS;

PLASMAS;

PLASMA; X-RAY SPECTROSCOPY;

EID: 30844444557     PISSN: 00224073     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.jqsrt.2005.05.057     Document Type: Article

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