Identification of spectral lines in the 500-1600 Å wavelength range of highly ionized Ne, Na, Mg, Ar, K, Ca, Ti, Cr, Mn, Fe, Co, and Ni emitted by flares (Te ≥ 3 ± 106 K) and their potential use in plasma diagnostics

Astrophysical Journal

Volumn 544, Issue 1 PART 1, 2000, Pages 508-521

  Feldman, U ^a   Curdt, W ^b   Landi, E ^b   Wilhelm, K ^b  

^a NAVAL RESEARCH LABORATORY   (United States)

^b MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

Author keywords

Line: identification; Sun: abundances; Sun: corona; Sun: flares; Sun: UV radiation

Indexed keywords

EID: 0034693512     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/317203     Document Type: Article

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