Low stiction low glide height head-disk interface for high-performance disk drives (invited)

Authors
Citation
Tc. Fu et S. Suzuki, Low stiction low glide height head-disk interface for high-performance disk drives (invited), J APPL PHYS, 85(8), 1999, pp. 5600-5605
Citations number
15
Categorie Soggetti
Apllied Physucs/Condensed Matter/Materiales Science
Journal title
JOURNAL OF APPLIED PHYSICS
ISSN journal
00218979 → ACNP
Volume
85
Issue
8
Year of publication
1999
Part
2B
Pages
5600 - 5605
Database
ISI
SICI code
0021-8979(19990415)85:8<5600:LSLGHH>2.0.ZU;2-O
Abstract
A brief historical review of the head-disk interface evolution is presented , and current limitations when facing stringent tribology requirements for high-density recording are addressed. The tribology performance of sliders with contact landing pads on the air bearing surfaces (the "padded slider'' ) was studied. Lightly mechanically textured disks, and laser zone-textured disks with shallow bumps (the "light LZT'') to reduce glide avalanche that were specially designed for padded sliders were used. When the smoother me chanically textured surface was applied, we observed inferior constant star t-stop (CSS) durability due to possible tribological degradation of the pad ded slider, and significant landing pad wear was observed on the slider aft er the CSS test. Rougher surfaces including the light LZT surface, however, were not as sensitive to tribological degradation of the padded slider as the smoother surface, and exhibited better CSS durability as well as less l anding pad wear after the test. Hence the optimization effort of padded sli der head/disk component design may be reduced if a light texture is applied on the CSS zone. The head-disk interface consisting of a padded slider on a light LZT can better meet the stringent tribology requirements for high d ensity recording needs and therefore it is proposed as an alternative to ra mp loading technology in the desktop/server-class disk drives. Hence the be tter-understood CSS technology is expected to be further extended into futu re high-performance disk drives. (C) 1999 American Institute of Physics. [S 0021-8979(99)31908-3].