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Micromagnetic Modeling of Recording on Discrete Track Perpendicular Media

机译:离散轨道垂直媒体记录的微磁模拟

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摘要

The rapidly increase in areal density of magnetic recording is placing very stringent requirements for signal to noise ratio (SNR). As the areal density grows, the track density increases and track pitch decreases substantially. As a result, the transition curvature and track edge noise becomes more severe. This imposes a barrier for improving SNR at higher densities. The discrete track media (DTM) [1,2,3] has been proposed to remedy the track edge effects through inter-track isolation, either physically or magnetically. The DTM is expected to have SNR advantages when compared to an equivalent conventional media with the same track density. In addition, the DTM might allow using recording heads with wider reader width and wider writer pole width. This might enable the drive manufacturers to use recording heads with relaxed head tolerances to improve manufacturing efficiency and yield. In this paper, the SNR performance of DTM is evaluated through micromagnetic simulation. The benefits of recording on DTM are discussed and compared to conventional media.
机译:磁记录的迅速增加是对信噪比(SNR)的非常严格的要求。随着地位密度的增长,轨道密度增加,并且轨道间距显着降低。结果,过渡曲率和轨道边缘噪声变得更严重。这迫使改善更高密度的SNR屏障。已经提出了离散轨道介质(DTM)[1,2,3]以通过物理或磁性地通过轨道间隔离来弥补轨道边缘效应。与具有相同轨道密度的等效传统介质相比,DTM预计将具有SNR优点。此外,DTM可能允许使用具有更宽读取器宽度和更宽的作者杆宽度的记录头。这可能使驱动制造商能够使用带有轻松的头部公差的记录头来提高制造效率和产量。在本文中,通过微磁性模拟评估DTM的SNR性能。与常规媒体进行讨论和比较DTM上记录的好处。

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