2006
DOI: 10.1109/tmag.2005.861768
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Direct measurement of magnetodynamics in a perpendicular recording system

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Cited by 12 publications
(3 citation statements)
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“…And the magnetic interaction between the writer pole of the perpendicular recording head and the SUL can result in technical problems concerning write processes, such as adjacent track erasure (ATE) [4], [5]. The direct observation of magnetic flux density and distribution in the SUL of perpendicular magnetic recording media provides highly useful information on the precise interaction between the SUL and a writer pole in the perpendicular magnetic recording system [6]. Further, the direct analysis of the magnetic flux magnitude and distribution in a nanoscale SUL is highly recommended because of the low SUL thickness and narrow writer pole width essential to achieve higher recording density [7], [8].…”
Section: Introductionmentioning
confidence: 99%
“…And the magnetic interaction between the writer pole of the perpendicular recording head and the SUL can result in technical problems concerning write processes, such as adjacent track erasure (ATE) [4], [5]. The direct observation of magnetic flux density and distribution in the SUL of perpendicular magnetic recording media provides highly useful information on the precise interaction between the SUL and a writer pole in the perpendicular magnetic recording system [6]. Further, the direct analysis of the magnetic flux magnitude and distribution in a nanoscale SUL is highly recommended because of the low SUL thickness and narrow writer pole width essential to achieve higher recording density [7], [8].…”
Section: Introductionmentioning
confidence: 99%
“…The interaction of recording head with soft underlayer (SUL) and return poles become very important in optimizing head and media at high data rates exceeding 1 Gb/s [1]- [3]. In order to calculate the dynamics of head field due to excitation by write coil field, full micromagnetic simulations are required [4]- [6].…”
Section: Introductionmentioning
confidence: 99%
“…T HE continuing advances in magnetic recording density and data rates require an ever more detailed understanding and control of the dynamic processes in magnetic write heads, recording media, and read heads. As the typical dimensions of the write pole of single-pole-type perpendicular recording heads shrink to about 100 nm and data rates exceed 1 Gb/s, the dynamic magnetization processes in the write pole and its interaction with the soft underlayer (SUL) and the return pole become very important [1]- [3]. In turn, the reduced size of the recording head makes it possible to perform fully micromagnetic simulations [4]- [6], which can model the intrinsic magnetization dynamics and the dynamic interaction with the SUL, which has to be considered part of the head because of its mirroring effect.…”
Section: Introductionmentioning
confidence: 99%