It appears you don't have support to open PDFs in this web browser. To view this file, Open with your PDF reader
Abstract
The magnetic properties of Co(10 Å)/NiO(40 Å)/Fe trilayer epitaxially grown on W(110) substrate were investigated with use of x-ray magnetic linear dichroism (XMLD) and x-ray magnetic circular dichroism (XMCD). We showed that magnetic anisotropy of Fe film that can be controlled by a thickness-driven spin reorientation transition is transferred via interfacial exchange coupling not only to NiO layer but further to ferromagnetic Co overlayer as well. Similarly, a temperature driven spin reorientation of Fe sublayer induces a reorientation of NiO spin orientation and simultaneous switching of the Co magnetization direction. Finally, by element specific XMCD and XMLD magnetic hysteresis loop measurements we proved that external magnetic field driven reorientation of Fe and Co magnetizations as well as NiO Néel vector are strictly correlated and magnetic anisotropy fields of Fe and Co sublayers are identical despite the different crystal structures.
You have requested "on-the-fly" machine translation of selected content from our databases. This functionality is provided solely for your convenience and is in no way intended to replace human translation. Show full disclaimer
Neither ProQuest nor its licensors make any representations or warranties with respect to the translations. The translations are automatically generated "AS IS" and "AS AVAILABLE" and are not retained in our systems. PROQUEST AND ITS LICENSORS SPECIFICALLY DISCLAIM ANY AND ALL EXPRESS OR IMPLIED WARRANTIES, INCLUDING WITHOUT LIMITATION, ANY WARRANTIES FOR AVAILABILITY, ACCURACY, TIMELINESS, COMPLETENESS, NON-INFRINGMENT, MERCHANTABILITY OR FITNESS FOR A PARTICULAR PURPOSE. Your use of the translations is subject to all use restrictions contained in your Electronic Products License Agreement and by using the translation functionality you agree to forgo any and all claims against ProQuest or its licensors for your use of the translation functionality and any output derived there from. Hide full disclaimer
Details
; Ślęzak, M. 1 ; Janus, W. 1 ; Nayyef, H. 1 ; Ślęzak, T. 1 ; Mandziak, A. 2 ; Zając, M. 2 ; Wilgocka-Ślęzak, D. 3 ; Menteş, T. O. 4 ; Jugovac, M. 4 ; Locatelli, A. 4
; Kozioł-Rachwał, A. 1 1 AGH University of Krakow, Faculty of Physics and Applied Computer Science, Krakow, Poland (GRID:grid.9922.0) (ISNI:0000 0000 9174 1488)
2 Jagiellonian University, National Synchrotron Radiation Centre SOLARIS, Krakow, Poland (GRID:grid.5522.0) (ISNI:0000 0001 2162 9631)
3 Polish Academy of Sciences, Jerzy Haber Institute of Catalysis and Surface Chemistry, Krakow, Poland (GRID:grid.413454.3) (ISNI:0000 0001 1958 0162)
4 Elettra – Sincrotrone Trieste, Basovizza, Trieste, Italy (GRID:grid.5942.a) (ISNI:0000 0004 1759 508X)




