Observation and modeling of high-n iron L-shell lines from intermediate ion stages

Astrophysical Journal

Volumn 496, Issue 2 PART I, 1998, Pages 1031-1043

  Wargelin, B J ^a,b   Beiersdorfer, P ^c   Liedahl, D A ^c   Kahn, S M ^a,d   Von Goeler, S ^e  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c LAWRENCE LIVERMORE NATIONAL LABORATORY   (United States)

^d Department of Earth and Environmental Sciences   (United States)

^e PRINCETON PLASMA PHYSICS LABORATORY   (United States)

Author keywords

Atomic data line: identification; Rays, gamma rays; Rays: general; Sun: X; X

Indexed keywords

EID: 0012628609     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/305410     Document Type: Article

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