001     87157
005     20250718144159.0
024 7 _ |2 ISSN
|a 1097-4539
024 7 _ |2 ISSN
|a 0049-8246
024 7 _ |2 WOS
|a WOS:000263882900010
024 7 _ |2 doi
|a 10.1002/xrs.1143
024 7 _ |a openalex:W2139088652
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037 _ _ |a PHPPUBDB-10840
041 _ _ |a English
082 _ _ |a 530
100 1 _ |0 P:(DE-HGF)0
|a Mukoyama, T.
|b 0
|e Corresponding author
110 1 _ |a DESY
|b Experiments with synchrotron radiation
245 _ _ |a Evolution of Satellite Lines
260 _ _ |a New York, NY [u.a.]
|b Wiley
|c 2009
300 _ _ |a 138-143
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|s 1481303620_26162
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|a Journal Article
440 _ 0 |0 PERI:(DE-600)1479999-6
|a X-Ray Spectrom.
|v 38
|x 0049-8246
500 _ _ |3 Converted on 2013-05-30 12:54
|a (c) John Wiley & Sons, Ltd. No post referee full text available.
500 _ _ |3 Converted on 2013-06-21 19:20
520 _ _ |a Evolution of the photoionized KLL Auger satellite line for 3$\mathit{d}$ transition metals was studied. The intensity ratio of the satellite line relative to the main $^{1}D_{2} (KL_{2}L_{3})$ 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.
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|a Uda, M.
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|a Köver, L.
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700 1 _ |0 P:(DE-HGF)0
|a Berenyi, Z.
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700 1 _ |0 P:(DE-H253)PIP1008428
|a Cserny, I.
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700 1 _ |0 P:(DE-H253)PIP1002684
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773 _ _ |0 PERI:(DE-600)1479999-6
|a 10.1002/xrs.1143
|g Vol. 38, p. 138-143
|p 138-143
|q 38<138-143
|t X-ray spectrometry
|v 38
|x 0049-8246
|y 2009
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