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Spectroscopy and atomic physics of highly ionized Cr, Fe, and Ni for tokamak plasmasThe paper considers the spectroscopy and atomic physics for some highly ionized Cr, Fe, and Ni ions produced in tokamak plasmas. Forbidden and intersystem wavelengths for Cr and Ni ions are extrapolated and interpolated using the known wavelengths for Fe lines identified in solar-flare plasmas. Tables of transition probabilities for the B I, C I, N I, O I, and F I isoelectronic sequences are presented, and collision strengths and transition probabilities for Cr, Fe, and Ni ions of the Be I sequence are given. Similarities of tokamak and solar spectra are discussed, and it is shown how the atomic data presented may be used to determine ion abundances and electron densities in low-density plasmas.
Document ID
19800039318
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Feldman, U. (Hulburt (E. O.) Center for Space Research Washington, DC, United States)
Doschek, G. A. (U.S. Navy, E. O. Hulburt Center for Space Research, Washington D.C., United States)
Cheng, C.-C. (U.S. Navy, E. O. Hulburt Center for Space Research, Washington, D.C.; Ball Corp. Boulder, Colo., United States)
Bhatia, A. K. (NASA Goddard Space Flight Center Laboratory for Astronomy and Astrophysics, Greenbelt, Md., United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1980
Publication Information
Publication: Journal of Applied Physics
Volume: 51
Subject Category
PLASMA PHYSICS
Distribution Limits
Public
Copyright
Other