Recent advances in the determination of atomic parameters for modeling K lines in cosmically abundant elements

Journal of Electron Spectroscopy and Related Phenomena

Volumn 184, Issue 3-6, 2011, Pages 170-173

  Quinet, P ^a,b   Palmeri, P ^a   Mendoza, C ^c   Bautista, M A ^d   Garcia, J ^e,f   Witthoeft, M C ^f   Kallman, T R ^f  

^a UNIVERSITY OF MONS   (Belgium)

^b UNIVERSITY OF LIÈGE   (Belgium)

^c INSTITUTO VENEZOLANO DE INVESTIGACIONES CIENTÍFICAS   (Venezuela)

^d WESTERN MICHIGAN UNIVERSITY   (United States)

^e CATHOLIC UNIVERSITY OF AMERICA   (United States)

^f NASA GODDARD SPACE FLIGHT CENTER   (United States)

Author keywords

Atomic processes; Auger rates; K lines; Photoionization; Radiative rates

Indexed keywords

ATOMIC PARAMETER; ATOMIC PROCESS; ATOMIC PROPERTIES; ATOMIC STRUCTURE; AUGER WIDTH; BREIT-PAULI R-MATRIX METHOD; HARTREE-FOCK; K-LINES; MULTICONFIGURATION DIRAC-FOCK METHOD; NI IONS; OPTICAL POTENTIAL; PHOTOABSORPTIONS; PHOTOIONIZATION CROSS SECTION; RADIATIVE RATES; SYSTEMATIC INVESTIGATIONS; THEORETICAL APPROACH;

ATOMS; AUGERS; IONS; NEON; PHOTOIONIZATION; RELATIVITY;

CRYSTAL ATOMIC STRUCTURE;

EID: 79957595683     PISSN: 03682048     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.elspec.2010.12.027     Document Type: Article

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