Micromagnetic modeling of low noise perpendicular media

2002 ◽  
Vol 91 (10) ◽  
pp. 8375 ◽  
Author(s):  
Alexander Shukh ◽  
Johannes van Ek
Keyword(s):  
Low Noise ◽  
Perpendicular Media ◽  
Micromagnetic Modeling

Micromagnetic Modeling of SNR Performance of Longitudinal and Perpendicular Media With Various Head/SUL Combinations

2004 ◽  
Vol 40 (4) ◽  
pp. 2555-2557 ◽  
Author(s):  
D.Z. Bai ◽  
A.F. Torabi ◽  
M. Benakli ◽  
M.L. Mallary ◽  
J.-G. Zhu
Keyword(s):  
Perpendicular Media ◽  
Micromagnetic Modeling

Low-noise CoCrPt/FeTaC double-layered perpendicular media with NiTaZr intermediate layer

2001 ◽  
Vol 235 (1-3) ◽  
pp. 59-63 ◽  
Author(s):  
K. Tanahashi ◽  
N. Shimizu ◽  
A. Kikukawa ◽  
Y. Takahashi ◽  
Y. Honda ◽  
...  
Keyword(s):  
Intermediate Layer ◽  
Low Noise ◽  
Perpendicular Media

Low noise Co/Pd multilayer perpendicular media with granular seed layer

2000 ◽  
Vol 36 (5) ◽  
pp. 2384-2386 ◽  
Author(s):  
H. Ohmori ◽  
A. Maesaka
Keyword(s):  
Seed Layer ◽  
Low Noise ◽  
Perpendicular Media

Micromagnetic modeling of discrete patterned perpendicular media

2003 ◽  
Vol 39 (5) ◽  
pp. 2326-2328 ◽  
Author(s):  
S. Haratani ◽  
A. Kaizu ◽  
I. Sato
Keyword(s):  
Perpendicular Media ◽  
Micromagnetic Modeling

Track Edge Noise Characteristics in Low Noise Longitudinal and Perpendicular Media

1997 ◽  
Vol 21 (S_2_PMRC_97_2) ◽  
pp. S2_265-268
Author(s):  
Chiaki Okuyama ◽  
Kenji Sato ◽  
Yuki Yoshida ◽  
Iwao Okamoto ◽  
Masayoshi Shinohara
Keyword(s):  
Low Noise ◽  
Perpendicular Media ◽  
Noise Characteristics

Low-noise CoCrPtO perpendicular media with improved resolution

2003 ◽  
Vol 39 (2) ◽  
pp. 668-672 ◽  
Author(s):  
E.M.T. Velu ◽  
S. Malhotra ◽  
G. Bertero ◽  
D. Wachenschwanz
Keyword(s):  
Low Noise ◽  
Perpendicular Media

Distribution of R- and S-Process Elements in the Galactic Halo

1988 ◽  
Vol 132 ◽  
pp. 501-506
Author(s):  
C. Sneden ◽  
C. A. Pilachowski ◽  
K. K. Gilroy ◽  
J. J. Cowan
Keyword(s):  
Heavy Element ◽  
Galactic Halo ◽  
Low Noise ◽  
Heavy Elements ◽  
Process Synthesis ◽  
Element Abundances ◽  
Halo Stars ◽  
Abundance Patterns ◽  
R Process ◽  
Process Elements

Current observational results for the abundances of the very heavy elements (Z>30) in Population II halo stars are reviewed. New high resolution, low noise spectra of many of these extremely metal-poor stars reveal general consistency in their overall abundance patterns. Below Galactic metallicities of [Fe/H] Ã −2, all of the very heavy elements were manufactured almost exclusively in r-process synthesis events. However, there is considerable star-to-star scatter in the overall level of very heavy element abundances, indicating the influence of local supernovas on element production in the very early, unmixed Galactic halo. The s-process appears to contribute substantially to stellar abundances only in stars more metal-rich than [Fe/H] Ã −2.

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