作者: C. W. Struck , W. H. Fonger
DOI: 10.1063/1.1659809
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摘要: Thermal quenchings of +3 rare‐earth line emissions were measured for excitation into the 4fn emitting states. These differ from corresponding reported by Wickersheim and Buchanan band‐gap excitation. For Tb+3, Tm+3, possible Pr+3, states are attributed, as in previously well‐established Eu+3 case, to thermally promoted crossovers Franck‐Condon‐shifted