TY  - JOUR
AU  - Mukoyama, T.
AU  - Uda, M.
AU  - Köver, L.
AU  - Berenyi, Z.
AU  - Cserny, I.
AU  - Drube, W.
AU  - DESY
TI  - Evolution of Satellite Lines
JO  - X-ray spectrometry
VL  - 38
SN  - 0049-8246
CY  - New York, NY [u.a.]
PB  - Wiley
M1  - PHPPUBDB-10840
SP  - 138-143
PY  - 2009
N1  - (c) John Wiley & Sons, Ltd. No post referee full text available.
AB  - Evolution of the photoionized KLL Auger satellite line for 3<i>d</i> transition metals was studied. The intensity ratio of the satellite line relative to the main <sup>1</sup>D<sub>2</sub> (KL<sub>2</sub>L<sub>3</sub>) diagram line was measured for Cu and Ni as a function of incident photon energy and the theoretical models based on the adiabatic approximation were fitted to the experimental data. The Thomas model, the Vatai model and the model of Roy et al. were considered. In addition, we modified the model of Roy et al. and developed a new model. Comparison of these four models was made and their difference was discussed.
LB  - PUB:(DE-HGF)16
UR  - <Go to ISI:>//WOS:000263882900010
DO  - DOI:10.1002/xrs.1143
UR  - https://bib-pubdb1.desy.de/record/87157
ER  -