New spectra of Fe XII to Fe XVIII and their isoelectronic sequences

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, , Citation B C Fawcett et al 1967 Proc. Phys. Soc. 90 863 DOI 10.1088/0370-1328/90/3/332

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1 Culham Laboratory, Nr. Abingdon, Berks

Dates

  1. Received 21 November 1966

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0370-1328/90/3/863

Abstract

The use of vacuum sparks and laser-produced plasmas has enabled many of the stronger transitions from these ions to be classified. New lines of Fe XII and XIII complete the classification of the intense members of the solar emission line group at 167 Å to 220 Å.

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