disk flutter
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2014 ◽  
Vol 50 (11) ◽  
pp. 1-4 ◽  
Author(s):  
Shinji Koganezawa ◽  
Tetsuki Yamamoto ◽  
Hiroshi Tani ◽  
Norio Tagawa

2014 ◽  
Vol 2014 (0) ◽  
pp. _S1620202--_S1620202-
Author(s):  
Shinji KOGANEZAWA ◽  
Tetsuki Yamamoto ◽  
Hiroshi Tani ◽  
Norio Tagawa

Author(s):  
J. Q. Mou ◽  
Q. D. Zhang ◽  
K. Sundaravadivelu ◽  
N. Y. Liu ◽  
E. H. Ong

In this paper, system level analysis is carried out for a functional HDD with two disks and four sliders operating at spindle speed of 15000 rpm. Full numerical models both for computational fluid dynamics (CFD) analysis and structural Finite Element Analysis (FEA) are developed. The flow induced vibrations of the sliders in all three directions, namely, off-track (X), down-track (Y) and out-of-plane direction (Z) are examined respectively. The numerical simulation results are compared and validated with the experimental results measured with a 3D laser Doppler vibrometer (LDV). Good agreements are observed for the vibrations in the three directions. The airflow patterns and characteristics of the flow induced vibration in HDD for three critical positions of the head gimbal assembly (HGA) parked at the disks identified as ID, MD and OD are investigated. The results reveal that the first slider from top has the highest flow induced vibrations in all the three directions due to the higher turbulent flow close to the top disk surface. Moreover, the results indicate that the slider vibration is interacted with the disk flutter in the HDD. Optimal designs of the HDD disk and air shroud are carried out to reduce the flow induced vibration of the slider, by suppressing the disk flutter and improving the turbulent flow in the HDD. It is demonstrated that significant reduction of flow induced slider vibration could be achieved with the optimal designs of the HDD.


2009 ◽  
Vol 15 (10-11) ◽  
pp. 1509-1513 ◽  
Author(s):  
Shinichi Ohtsuka ◽  
Shinji Koganezawa ◽  
Takeyori Hara ◽  
Kei Funabashi ◽  
Takuji Matsuzawa

2008 ◽  
Vol 08 (01) ◽  
pp. 41-60 ◽  
Author(s):  
XINGZHE WANG ◽  
X. Y. HUANG

In this paper, the dynamic stability of a disk rotating in air has been modeled and analyzed numerically as well as observed from experiments. A simple expression on the aerodynamic loading acting on the rotating disk is applied in the modeling, and the dynamic stability results of the disks are evaluated based on the eigenvalues for the vibration modes. The disk critical speeds and the flutter speeds are calculated and compared with the results from experiments, which are conducted on two steel disks with different diameters and thicknesses. The modeling predicts that the rotating disk flutter starts with the mode (0, 3)B, which agrees with the results reported in the literature and the observation in the present experimental study.


2006 ◽  
Vol 129 (3) ◽  
pp. 368-375 ◽  
Author(s):  
Shigenori Takada ◽  
Norio Tagawa ◽  
Atsunobu Mori ◽  
Yoshiaki Mizoh ◽  
Masaru Nakakita

It is important to clarify the characteristics of flow-induced vibrations in hard disk drives in order to achieve an ultrahigh magnetic recording density. In particular, it is necessary to reduce the flow-induced disk vibrations referred to as disk flutter. This paper describes the correlation between the disk vibration amplitude and the pressure fluctuation between a pair of high-speed corotating disks. It also reveals the effects of the arm thickness and arm shape on the disk vibrations and the static pressure between the disks. The disk vibrations were measured using a laser Doppler vibrometer (LDV). The static pressure downstream of the arm between a pair of narrow disks was measured by a method in which a side-hole needle was used as a measurement probe. In addition, the direction of air flow along the trailing edge of the arm was measured using a hot-wire anemometer. The experimental results revealed that the arm inserted between the disks suppresses the disk vibrations. However, the shape and thickness of the arm did not quantitatively affect the disk vibrations. The root-mean-square (RMS) static pressure fluctuation downstream of the arm decreased remarkably, whereas the mean static pressure increased when the arm was inserted between the disks. Furthermore, the circumferential variations in both the RMS and mean static pressures reduced when the arm was inserted. Therefore, it is suggested that the disk vibrations are excited by an increase in the static pressure fluctuation, mean dynamic pressure, and circumferential variation in the static pressure between the disks. Consequently, the disk vibrations can be suppressed by inserting the arm or a spoiler.


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