Time-resolved scanning Kerr microscopy of flux beam formation in hard disk write heads

被引:4
作者
Valkass, Robert A. J. [1 ]
Spicer, Timothy M. [1 ]
Parra, Erick Burgos [1 ]
Hicken, Robert J. [1 ]
Bashir, Muhammad A. [2 ]
Gubbins, Mark A. [2 ]
Czoschke, Peter J. [3 ]
Lopusnik, Radek [3 ]
机构
[1] Univ Exeter, Dept Phys & Astron, Stocker Rd, Exeter EX4 4QL, Devon, England
[2] Seagate Technol, Res & Dev, 1 Disc Dr,Springtown Ind Estate, Derry BT48 0BF, North Ireland
[3] Seagate Technol, Recording Heads Operat, 7801 Comp Ave South, Bloomington, MN 55435 USA
关键词
MAGNETIZATION DYNAMICS; POLE;
D O I
10.1063/1.4954018
中图分类号
O59 [应用物理学];
学科分类号
摘要
To 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 devices, as well as being relevant to other magnetic devices. Published by AIP Publishing.
引用
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页数:7
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