Abstract
The portion of pair emission in ruby which is due to energy transfer from single ions has been continously recorded as a function of an external magnetic field (in the range 0 - 100 kg) at various temperatures (2–77 K). 3rd and 4th neighbours pairs have been investigated (N1 and N2 emission lines respectively).
© 1984 Optical Society of America
PDF ArticleMore Like This
R. Buisson
TuH1 International Conference on Luminescence (ICOL) 1984
A. Monteil, E. Duval, A. Attar, and G. Viliani
WE8 International Conference on Luminescence (ICOL) 1984
A.A. Kaplyanskii, S.A. Basoon, and S.P. Feofilov
WE6 International Conference on Luminescence (ICOL) 1984