Microstructure and Recording Noise of Thin Film Longitudinal Media

1991 ◽  
Vol 232 ◽  
Author(s):  
Tadashi Yogi ◽  
Thao A. Nguyena ◽  
Steven E. Lambert ◽  
Grace L. Gorman ◽  
Gil Castillo

ABSTRACTThe magnetic and recording characteristics of Co-based thin film media are strongly influenced by microstructure. The media microstructural characteristics, in turn, depend on sputtering conditions of underlayers and magnetic layers. The role of Cr underlayer thickness and sputtering pressure have been reported previously. The present work examines the growth morphology and recording properties of a CoPtCr alloy on Cr underlayers where the deposition conditions such as sputtering pressure and rf bias were independently varied for the Cr underlayer and the magnetic layer. We find that the growth morphology of the magnetic layer is governed primarily by the deposition condition of the Cr underlayer. In particular, increased sputtering pressure for the Cr underlayer produces columnar morphology which induces isolation of the grains in the magnetic layer. This results in a significant reduction in the recording noise due to reduced intergrain exchange coupling. On the other hand, the application of ff bias during the deposition of the magnetic layer promotes more continuous magnetic grains, thereby increasing the recording noise. The observed trends in microstructure and recording noise can be understood qualitatively in terms of Thornton's microstructure diagram and the competition between micromorphological roughness and adatom mobility during the film growth.

Metals ◽  
2018 ◽  
Vol 9 (1) ◽  
pp. 12 ◽  
Author(s):  
Hayk Khachatryan ◽  
Sung-Nam Lee ◽  
Kyoung-Bo Kim ◽  
Moojin Kim

In this study, we deposited aluminum (Al) films of different thicknesses on steel substrate and examined their phase, microstructure, and film growth process. We estimated that films of up to 30 nm thickness were mainly amorphous in nature. When the film thickness exceeded 30 nm, crystallization was observed. The further increase in film thickness triggered grain growth, and the formation of grains up to 40 nm occurred. In such cases, the Al film had a cross-grained structure with well-developed primary grains networks that were filled with small secondary grains. We demonstrated that the microstructure played a key role in optical properties. The films below 30 nm showed higher specular reflection, whereas thicker films showed higher diffuse reflections.


2006 ◽  
Vol 18 (32) ◽  
pp. S1771-S1776 ◽  
Author(s):  
James Birrell ◽  
J E Gerbi ◽  
O A Auciello ◽  
J A Carlisle

2009 ◽  
Vol 19 (12) ◽  
pp. 1962-1970 ◽  
Author(s):  
Ajay Virkar ◽  
Stefan Mannsfeld ◽  
Joon Hak Oh ◽  
Michael F. Toney ◽  
Yih Horng Tan ◽  
...  

1997 ◽  
Vol 56 (2) ◽  
pp. 1522-1530 ◽  
Author(s):  
Chung-Yu Mou ◽  
J. W. P. Hsu

1999 ◽  
Vol 110 (24) ◽  
pp. 12151-12160 ◽  
Author(s):  
Thomas R. Mattsson ◽  
Greg Mills ◽  
Horia Metiu

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