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A Study of the Head Disk Interface in Heat Assisted Magnetic Recording - Energy and Mass Transfer in Nanoscale

机译:热辅助磁记录中磁头磁盘界面的研究-纳米级的能量和质量传递

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摘要

The hard disk drive (HDD) is still the dominant technology in digital data storage due to its cost efficiency and long term reliability compared with other forms of data storage devices. The HDDs are widely used in personal computing, gaming devices, cloud services, data centers, surveillance, etc. Because the superparamagnetic limit of perpendicular magnetic recording (PMR) has been reached at the data density of about 1 Tb/in2 , heat assisted magnetic recording (HAMR) is being pursued and is expected to help increase the areal density to over 10 Tb/in2 in HDDs in order to fulfill the future worldwide data storage demands.;In HAMR, the magnetic media is heated locally (∼50nm x 50nm) and momentarily (∼10ns) to its Curie temperature (∼750K) by a laser beam. The laser beam is generated by a laser diode (LD) and focused by a near field transducer (NFT). But the energy and mass transfer at high temperature from the laser heating can cause potential reliability issues. The design temperature of the NFT is much lower than the media's Curie temperature. However, the distance between the NFT and the media is less than 10nm. As a result, the heat can flow back from the media to the NFT, which is called the back-heating effect. This can cause undesired additional temperature increase on the NFT, shortening its lifetime. Additionally, depletion, evaporation and degradation can happen on the lubricant and the carbon overcoat (COC) layer of the media. The material can transfer from the media to the head at high temperature and cause solid contamination on the head, adversely affecting its reliability.;Since the laser heating in HAMR happens at nanoscale spatially and temporally, it is difficult to measure experimentally. In this dissertation, a comprehensive experimental stage, called the Computer Mechanics Laboratory (CML)-HAMR stage, was built to study different aspects of HAMR systems, including the heat and mass transfer in the head-disk interface during laser heating. The CML-HAMR stage includes an optical module, a spinstand module and a signal generation/acquisition module. And it can emulate the HAMR scenario.;The head's temperature was measured during the laser heating using the stage and heads with an embedded contact sensor (ECS). It was estimated, based on a linear extrapolation, that the ECS temperature rise is 139K, 132K, 127K and 122K when the disk is heated to the Curie temperature (∼750K) and the head-disk clearance is 0nm, 1nm, 2nm and 3nm, respectively. The heating effect of the ECS was also studied and a related heat transfer experiment was performed. The normalized ECS self heating temperature rise, an indicator of the heat transfer in the head-disk interface (HDI), was measured. It was concluded that the heat transfer coefficient across the HDI strongly depends on the width of the gap size, especially when the gap size is smaller than 1nm.;The head disk interaction during the laser heating was studied using a waveguide head, i.e., a HAMR head without the NFT. It showed that the laser heating can cause head surface protrusion. This lowers the fly-height (FH) and results in early touchdown (TD). It was shown that the ratio of touchdown power (TDP) change to the laser current is 0.3mW/mA. The dynamics of the head also changes during the laser heating. It was found that the magnitude of the 1st-pitch-mode vibration on the head increases over time both in short term and long term. The accumulation of material transferred to the head was also investigated. It was found that the solid contamination caused by the laser heating forms in the center of the waveguide. The round-shaped contamination formed on the head surface after laser heating.;Finally the disk lubricant reflow after laser heating was studied. In the experiment, a beam of free space laser shines on the rotating disk at different laser powers, disk rotating speeds and repetitions. Then the disk was examined by an optical surface analyzer (OSA). It was found that 80% of the displaced lubricant recovers within 20 minutes. A simulation was also performed. The experiments and the simulation are in good agreement.
机译:与其他形式的数据存储设备相比,硬盘驱动器(HDD)的成本效率和长期可靠性仍然是数字数据存储中的主要技术。 HDD广泛用于个人计算,游戏设备,云服务,数据中心,监视等。由于垂直磁记录(PMR)的超顺磁极限已达到大约1 Tb / in2的数据密度,因此热辅助磁记录(HAMR)正在研究中,有望帮助将HDD中的面密度提高到10 Tb / in2以上,以满足未来全球范围内的数据存储需求。;在HAMR中,磁性介质被局部加热(〜50nm x 50nm )并通过激光束暂时(〜10ns)达到其居里温度(〜750K)。激光束由激光二极管(LD)产生,并由近场换能器(NFT)聚焦。但是,激光加热导致的高温下的能量和质量传递会引起潜在的可靠性问题。 NFT的设计温度远低于介质的居里温度。但是,NFT与介质之间的距离小于10nm。结果,热量可以从介质流回NFT,这称为回热效应。这可能会导致NFT出现不希望的额外温度升高,从而缩短其使用寿命。此外,介质的润滑剂和碳涂层(COC)层上可能会发生消耗,蒸发和降解。该材料会在高温下从介质转移到头部,并在头部造成固体污染,从而影响其可靠性。由于HAMR中的激光加热在空间和时间上都是纳米级的,因此很难通过实验进行测量。本文建立了一个综合的实验阶段,称为计算机力学实验室(CML)-HAMR阶段,以研究HAMR系统的各个方面,包括激光加热过程中磁头-磁盘界面的传热和传质。 CML-HAMR平台包括一个光学模块,一个自旋支架模块和一个信号生成/获取模块。并且它可以模拟HAMR场景。头的温度是在激光加热期间使用载物台和带有嵌入式接触传感器(ECS)的头测量的。根据线性外推法估计,当将磁盘加热到居里温度(〜750K)并且磁头磁盘间隙为0nm,1nm,2nm和3nm时,ECS温升为139K,132K,127K和122K。 , 分别。还研究了ECS的加热效果,并进行了相关的传热实验。测量了标准化的ECS自加热温度升高,该温度升高是磁头-磁盘界面(HDI)中热传递的指标。结论是,HDI上的传热系数在很大程度上取决于间隙尺寸的宽度,尤其是当间隙尺寸小于1nm时。;使用波导头研究了激光加热期间的头盘相互作用,即没有NFT的HAMR头。结果表明,激光加热会导致头部表面突出。这会降低飞行高度(FH),并导致早期着陆(TD)。结果表明,接地功率(TDP)变化与激光电流的比率为0.3mW / mA。在激光加热过程中,头部的动态也会发生变化。结果发现,无论是短期还是长期,头部的第一音调模式振动的幅度都随时间增加。还研究了转移到头部的材料的积累。发现由激光加热引起的固体污染在波导的中心形成。激光加热后在头部表面形成了圆形污染。最后,研究了激光加热后磁盘润滑剂的回流情况。在实验中,自由空间激光束以不同的激光功率,磁盘旋转速度和重复频率照射在旋转磁盘上。然后通过光学表面分析仪(OSA)检查磁盘。发现80%的置换润滑剂在20分钟内恢复。还进行了模拟。实验与仿真吻合良好。

著录项

  • 作者

    Wu, Haoyu.;

  • 作者单位

    University of California, Berkeley.;

  • 授予单位 University of California, Berkeley.;
  • 学科 Mechanical engineering.
  • 学位 Ph.D.
  • 年度 2018
  • 页码 115 p.
  • 总页数 115
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

  • 入库时间 2022-08-17 11:40:03

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