Temperature-sensitive line ratios of the lithium-like ion O VI

Details Temperature-sensitive line ratios of the lithium-like ion O VI Temperature-sensitive line ratios of the lithium-like ion O VI

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..136..111h&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 136, Nov. 1991, p. 111-116.

Physics

1

Electron Energy, Emission Spectra, Lithium, Oxygen Ions, Oxygen Spectra, Solar Corona, High Temperature Plasmas, Isoelectronic Sequence, Temperature Effects

Scientific paper

The intensity ratios of emission lines from the lithium-like ion O VI are calculated as a function of electron temperature using recent computations of collision strengths by Zhang, Sampson, and Fontes (1990). The line ratios are strongly dependent on temperature and are appropriate as a diagnostic of hot thin plasmas such as in the solar transition region and corona.

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