传统和瓦式磁记录对读写器的依赖

S. Granz, C. Rea, Cathy Jackson, M. Gubbins, G. Ju, J. Thiele, T. Rausch
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引用次数: 4

摘要

热辅助磁记录(HAMR)是下一代硬盘驱动技术,可实现持续且显著的面密度增长[1]。随着轨道间距继续缩小,HAMR阅读器必须继续扩大规模。在高磁道密度下,当前读写器技术的可扩展性受到极大挑战[2]-[3]。随着面密度的显著增长,读卡器宽度必须以高信噪比(SNR)减小,以避免相邻轨道的侧读取。通常,阅读器宽度和信噪比之间存在权衡[4]-[5]。为了使HAMR面密度继续扩大,有必要在不降低信噪比的情况下减小读取器宽度。传统的阅读器头媒体间距(HMS)减小和阅读器宽度缩放可能不足以提高高音轨的阅读器分辨率。在本文中,我们比较了HAMR传统磁记录(CMR)和HAMR瓦式磁记录(SMR)在不同读写器间隙下与集成HAMR读写器和交叉测试(CT)窄高信噪比读写器的面密度能力(ADC)。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Heat Assisted Magnetic Recording Dependence on Reader for Conventional and Shingled Magnetic Recording
Heat Assisted Magnetic Recording (HAMR) is the next generation hard disk drive technology which enables continued and significant areal density growth [1]. As the track pitch continues to scale down, the HAMR reader must continue to scale. The scalability of the current reader technology is greatly challenged at high track densities [2]–[3]. With significant growth in areal density, the reader width must reduce with high signal to noise ratio (SNR) to avoid side reading from adjacent tracks. Typically, there is a tradeoff between reader width and SNR [4]–[5]. For HAMR areal density to continue to scale, innovations to enable reader width reduction without SNR degradation are necessary. Traditional reader head media spacing (HMS) reduction and reader width scaling may not be enough to improve the reader resolution for high track pitches. In this paper, we compare the areal density capability (ADC) of HAMR Conventional Magnetic Recording (CMR) and HAMR Shingled Magnetic Recording (SMR) at various reader clearances with integrated HAMR readers and cross tested (CT) narrow high SNR readers.
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