Please use this identifier to cite or link to this item: http://hdl.handle.net/10995/92568
Title: Magnetic microstructure of the Finemet-type thin films
Authors: Mikhalitsyna, E.
Soboleva, E.
Kataev, V.
Kulesh, N.
Lhderanta, E.
Issue Date: 2019
Publisher: Institute of Physics Publishing
Citation: Magnetic microstructure of the Finemet-type thin films / E. Mikhalitsyna, E. Soboleva, V. Kataev, N. Kulesh, et al.. — DOI 10.1088/1742-6596/1389/1/012114 // Journal of Physics: Conference Series. — 2019. — Vol. 1. — Iss. 1389. — 12114.
Abstract: Fe73.9Cu1Nb3Si13.2B8.9 thin films were deposited on the glass substrates by means of ion-plasma radio frequency sputtering. Heat treatment at temperatures of 350, 400 and 450 C was performed for 30 minutes in order to control thin film structural state. The X-ray powder diffraction showed that the crystallization of α-Fe(Si) nanograins took place at the temperature of 420 C whilst the other samples stayed in the amorphous state. The magnetic microstructure of the Fe73.9Cu1Nb3Si13.2B8.9 films was discussed in the framework of random anisotropy model and law of approach of magnetization to saturation. The parameters of magnetic microstructure were determined, and relations between structure and macroscopic magnetic properties were interpreted by means of magnetic microstructure analysis. © Published under licence by IOP Publishing Ltd.
Keywords: AMORPHOUS SILICON
COPPER COMPOUNDS
IRON COMPOUNDS
MICROSTRUCTURE
NIOBIUM COMPOUNDS
SATURATION MAGNETIZATION
SILICON COMPOUNDS
SPUTTERING
SUBSTRATES
THIN FILMS
X RAY POWDER DIFFRACTION
AMORPHOUS STATE
CONTROL THIN FILM
GLASS SUBSTRATES
LAW OF APPROACHES
MAGNETIC MICROSTRUCTURES
RADIO FREQUENCY SPUTTERING
RANDOM ANISOTROPY MODELS
STRUCTURAL STATE
BORON COMPOUNDS
URI: http://hdl.handle.net/10995/92568
Access: info:eu-repo/semantics/openAccess
SCOPUS ID: 85076724795
WOS ID: 000562319800114
PURE ID: 11760921
ISSN: 1742-6588
DOI: 10.1088/1742-6596/1389/1/012114
metadata.dc.description.sponsorship: № 18-32-00221
№ 02.A03.21.0006
The study was funded in part by RFBR according to the research project № 18-32-00221 (mol_a). The work was supported by Act 211 Government of the Russian Federation, contract № 02.A03.21.0006.
Appears in Collections:Научные публикации, проиндексированные в SCOPUS и WoS CC

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