An Experiment Study of Head-to-Media Spacing Sensitivity in Ultra-high Density Magnetic Recording Systems

dc.contributor.authorPichet Nhunork
dc.contributor.authorChanon Warisarn
dc.contributor.authorDamrongsak Tongsomporn
dc.date.accessioned2025-07-21T05:56:34Z
dc.date.issued2016-01-01
dc.description.abstractThe decrease in flying height due to the higher recording areal density of hard disk drives (HDDs) has had a huge impact on data storage technology. The head protrusion that induced by ambient temperature can further reduce flying clearance by a few nanometers. However, the head-disk interface reliability should be also emphasized; since when the head flies too close to the media, the recording head may be burnished. To investigate the head-to-media spacing sensitivity, we use the spin stand tester and analyze the sensitivity through the measurement of overwrite (OVW), micro-track profile (MTP), and signal-to-noise ratio (SNR). The experiment results imply the significant relationship between the OVW and the heater-induced writer protrusion (H-IWP). Furthermore, we verify that the properly reduction of head-to-media spacing can also enhance the both of writability and readability.
dc.identifier.doi10.1016/j.procs.2016.05.048
dc.identifier.urihttps://dspace.kmitl.ac.th/handle/123456789/5536
dc.subjectFlying height
dc.subjectPatterned media
dc.subjectArea density
dc.subjectOptical disc
dc.subjectRecording media
dc.subjectSIGNAL (programming language)
dc.subjectRecording head
dc.subject.classificationMagnetic properties of thin films
dc.titleAn Experiment Study of Head-to-Media Spacing Sensitivity in Ultra-high Density Magnetic Recording Systems
dc.typeArticle

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