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@ARTICLE{Mukoyama:87157,
      author       = {Mukoyama, T. and Uda, M. and Köver, L. and Berenyi, Z. and
                      Cserny, I. and Drube, W. and DESY},
      title        = {{E}volution of {S}atellite {L}ines},
      journal      = {X-ray spectrometry},
      volume       = {38},
      issn         = {0049-8246},
      address      = {New York, NY [u.a.]},
      publisher    = {Wiley},
      reportid     = {PHPPUBDB-10840},
      pages        = {138-143},
      year         = {2009},
      note         = {(c) John Wiley $\&$ Sons, Ltd. No post referee full text
                      available.},
      abstract     = {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.},
      cin          = {HASYLAB(-2012)},
      ddc          = {530},
      cid          = {$I:(DE-H253)HASYLAB_-2012_-20130307$},
      pnm          = {DORIS Beamline BW2 (POF1-550)},
      pid          = {G:(DE-H253)POF1-BW2-20130405},
      experiment   = {EXP:(DE-H253)D-BW2-20150101},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:000263882900010},
      doi          = {10.1002/xrs.1143},
      url          = {https://bib-pubdb1.desy.de/record/87157},
}