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dc.contributor.authorValkass, Robert Alexander James
dc.contributor.authorSpicer, Timothy M
dc.contributor.authorBurgos Parra, Erick
dc.contributor.authorHicken, Robert James
dc.contributor.authorBashir, Muhammad A
dc.contributor.authorGubbins, Mark A
dc.contributor.authorCzoschke, Peter J
dc.contributor.authorLopusnik, Radek
dc.date.accessioned2016-06-27T15:11:43Z
dc.date.issued2016
dc.description.abstractTo meet growing data storage needs, the density of data stored on hard disk drives must increase. In pursuit of this aim the magnetodynamics of the hard disk write head must be characterized and understood, particularly the process of “flux beaming”. In this study, seven different configurations of perpendicular magnetic recording (PMR) write heads were imaged using time-resolved scanning Kerr microscopy, revealing their detailed dynamic magnetic state during the write process. It was found that the precise position and number of driving coils can significantly alter the formation of flux beams during the write process. These results are applicable to the design and understanding of current PMR and next-generation heat-assisted magnetic recording (HAMR) devices, as well as being relevant to other magnetic devices.en_GB
dc.description.sponsorshipThe authors gratefully acknowledge financial support from the Seagate Plan.en_GB
dc.identifier.citationVol. 119: 233903en_GB
dc.identifier.doi10.1063/1.4954018
dc.identifier.urihttp://hdl.handle.net/10871/22269
dc.language.isoenen_GB
dc.publisherAmerican Institute of Physics (AIP)en_GB
dc.relation.urlhttp://hdl.handle.net/10871/21108en_GB
dc.subjectdomain wallsen_GB
dc.subjectcoilsen_GB
dc.subjectspatial dimensionsen_GB
dc.subjectmagnetic storage devicesen_GB
dc.subjecttime solved imagingen_GB
dc.titleTime resolved scanning Kerr microscopy of flux beam formation in hard disk write headsen_GB
dc.typeArticleen_GB
dc.date.available2016-06-27T15:11:43Z
dc.identifier.issn1089-7550
dc.descriptionThis is the author accepted manuscript. The final version is available from the publisher via the DOI in this record.en_GB
dc.descriptionThe underlying research dataset supporting this publication is available under a Creative Commons Attribution-ShareAlike 4.0 International License (https://creativecommons. org/licenses/by-sa/4.0/) and can be publicly accessed in Open Research Exeter via the following persistent identifier: http://hdl.handle.net/10871/21108.en_GB
dc.identifier.journalJournal of Applied Physicsen_GB


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