Abstract
The average L-shell fluorescence yields in Zr, Nb, Mo, Ag, Cd, In, Sn and I have been measured using photoionization for creating the vacancies. The present results are found to agree well with those calculated using the values of L-subshell fluorescence yields and Coster-Kronig yields of Krause et al., but are lower than the only available experimental results of Lay. To the best of our knowledge, the values in Nb, Cd, In and I are reported for the first time.
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