A survey of current coronal visible line identifications
暂无分享,去创建一个
[1] W. Deutschman,et al. Additional resonance lines of highly ionized sulfur, chlorine, argon, and potassium. , 1967 .
[2] F. Orrall,et al. A Photometric Study of the Continuum and Seventeen Emission Lines in the Inner Solar Corona. , 1962 .
[3] L. Aller. Astrophysics. The Atmospheres of the Sun and Stars , 1954 .
[4] H. Klüber. The Solar Corona , 1966, Nature.
[5] W. Deutschman,et al. New inner-shell resonance lines in highly ionized sulfur and chlorine. , 1966 .
[6] F. Rohrlich,et al. Highly Ionized Atoms: the Configurations S^{2}P^{n} (n = 1, 2, 4, 5). , 1963 .
[7] R. Garstang. Energy levels and transition probabilities in p4 and p4 configurations , 1951 .
[8] B. Lyot,et al. Preliminary Note on Measures of Coronal Emission Lines Observed at Total Solar Eclipse, February 25, 1952, by , 1955 .
[9] R. Garstang. ON THE CORONAL LINES λλ 5445, 5694, AND 4086. , 1952 .
[10] Donald E. Billings,et al. A Guide to the Solar Corona , 2013 .