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

MPS-Authors
http://pubman.mpdl.mpg.de/cone/persons/resource/persons103872

Curdt,  W.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons104045

Landi,  E.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons104293

Wilhelm,  K.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Feldman, U., Curdt, W., Landi, E., & Wilhelm, K. (2000). Identification of spectral lines in the 500-1600 Å wavelength range of highly ionized Ne, Na, Ar, K, Ca, Ti, Cr, Mn, Fe, Co, and Ni emitted by flares (Te gt;= 3 × 106 K) and their potential use in plasma diagnostics. Astrophysical Journal, 544, 508-521.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-E118-D
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