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| VOLUME 22 (1975) | ISSUE 4 |
PAGE 245
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Possibility of observing coronal spectral lines in a laboratory plasma
Shcheglov D. A.
The factors that determine the possibility of registration, under laboratory conditions, of forbidden lines observable in the spectrum of the solar corona are discussed. Certain results of spectroscopic measurements in the "Tokamak-4" installations are interpreted as observation of the "green line" of the ion Fe XIV.
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![](/ps/1523/article_23310_800_head.png "The factors that determine the possibility of registration, under laboratory conditions, of forbidden lines observable in the spectrum of the solar corona are discussed. Certain results of spectroscopic measurements in the "Tokamak-4" installations are interpreted as observation of the "green line" of the ion Fe XIV.")