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Energy Barrier Analysis of High Density Hamr Simulations

机译:高密度HAMR模拟的能量屏障分析

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Some form of heat assistance is likely to be required to achieve >3Tbpsi recording density and continue the long progression of capacity growth of magnetic recording in hard disk drives. To provide useful component design guidance, micromagnetic simulations of heat assisted magnetic recording (HAMR) must include estimates of the areal density of the recording system. In earlier work prepared for Intermag 2020 we investigated the influence of both near-field transducer and medium design on areal density. Exploring a range of medium and NFT designs we demonstrated that once the thermal gradient of the head & medium system is sufficient, the achievable jitter (and hence linear density) is governed by the magnetic properties of the medium. Including read-back parameters, we outlined requirements for HAMR recording systems capable of achieving > 2 Tbpsi in hard disk drives with product margins [1].
机译:可能需要某种形式的热辅助来实现> 3TBPSI记录密度,并在硬盘驱动器中继续磁记录的能力生长的长进展。为了提供有用的组件设计指导,热辅助磁记录(HAMR)的微观仿真必须包括记录系统的面密度的估计。在为intermag 2020准备的早期工作中,我们调查了近场传感器和中型设计对区域密度的影响。探索一系列培养基和NFT设计,我们证明了一旦头部和介质系统的热梯度就足够了,可实现的抖动(并且因此线性密度)由介质的磁性计算。包括读回参数,我们对HAMR录制系统的要求概述了能够在具有产品边缘的硬盘驱动器中实现> 2 TBPSI [1]。

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