Fe XIX transitions within the N = 2 complex

Details Fe XIX transitions within the N = 2 complex Fe XIX transitions within the N = 2 complex

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...150..246l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 150, no. 2, Sept. 1985, p. 246-250. SERC-supported research.

Astronomy and Astrophysics

Astrophysics

22

Electron Transitions, Iron, Plasma Spectra, Solar Flares, Solar Spectra, Atomic Energy Levels, Emissivity, Line Spectra, Oscillator Strengths, Tokamak Devices, Transition Probabilities

Scientific paper

The authors calculate the atomic data necessary for the interpretation of the Fe XIX spectra emitted by solar flare and tokamak plasmas. They consider the transitions between the 2s22p4, 2s2p5,and 2p6 configurations. Some of the Fe XIX lines are potentially useful for determining electron density, and for one XUV flare spectrum they find evidence to indicate an electron density in excess of 1013cm-3.

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