On the Identification of Ca XV and A XIV in the Solar Corona
Open Access
- 1 December 1954
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 114 (6) , 700-703
- https://doi.org/10.1093/mnras/114.6.700
Abstract
The interpretation of the coronal wave-lengths λ 5694 and λ 5446 as transitions in Ca XV is shown to be compatible with known isoelectronic data on level intervals. The original suggestion concerning A XIV is revised and the identification transferred from λ 4359 to the new coronal line λ 4412.Keywords
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