Physical Review · 1941 · 66 citations · 8 references
Natural SciencesPhysicsNuclear PhysicsSpeciationUltraviolet AstronomyFine StructureSpectral InterpretationGround State PropertiesLevelsLimitsLine Emission SpectraSpark Emission SpectroscopySpectral Line Structure
Structure of the spectrum. The strongest lines of Eu II arise from transitions based on the ground-level of Eu III, ${f}^{7}^{8}S^{\mathrm{o}}$. The lowest terms are ${f}^{7}s^{9}S^{\mathrm{o}}$, $^{7}S^{\mathrm{o}}$. Next come ${f}^{7}d^{9}D^{\mathrm{o}}$, $^{7}D^{\mathrm{o}}$. Numerous levels, combining with these terms, arise from ${f}^{6}{s}^{2}$, ${f}^{6}\mathrm{sd}$, and ${f}^{8}$. The number of levels identified is 156; of lines classified, 467. All the stronger lines are included. Unclassified lines. About 2000 lines remain unclassified. They probably arise from transitions between levels based upon higher limits in the ${f}^{7}$ configuration of Eu III. Ionization potential. Series of three consecutive $^{9}S^{\mathrm{o}}$ and $^{7}S^{\mathrm{o}}$ terms give the value 11.21 volts. Zeeman effect. Patterns for 459 lines, measured at the Massachusetts Institute of Technology, with a field of 87,850 gauss, are tabulated. The $g$ values for 118 levels have been determined. Those for the low levels agree with theory; the higher levels are much perturbed. Patterns for a few lines of Eu I and Eu III are given. The latter confirm that the ground state is $^{8}S^{\mathrm{o}}$.
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Henry Norris Russell, Arthur S. King · The Astrophysical Journal · 1939 · 49 citations
Analysis of the Spectrum of Singly Ionized Samarium
Walter Albertson · The Astrophysical Journal · 1936 · 45 citations · Full text