New spectra of Fe XII to Fe XVIII and their isoelectronic sequences
B C Fawcett; A H Gabriel; P A H Saunders; B C Fawcett; Culham Laboratory, Nr. Abingdon, Berks; A H Gabriel; Culham Laboratory, Nr. Abingdon, Berks; P A H Saunders; Culham Laboratory, Nr. Abingdon, Berks
Журнал:
Proceedings of the Physical Society
Дата:
1967-03-01
Аннотация:
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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